634 Supergiants PPTs View free & download

Blue Supergiants as a Tool for Extragalactic Distances - Blue Supergiants as a Tool for Extragalactic Distances

Blue Supergiants as a Tool for Extragalactic Distances

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Atmospheres, pulsation, and massloss of AGB stars and supergiants - Atmospheres, pulsation, and massloss of AGB stars and supergiants

Atmospheres, pulsation, and massloss of AGB stars and supergiants

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Metallicity Dependence of Winds from Red SuperGiants and Asymptotic Giant Branch Stars PowerPoint PPT Presentation

Metallicity Dependence of Winds from Red SuperGiants and Asymptotic Giant Branch Stars - Jacco van Loon. Keele University. Dust wind structure. Radiative equilibrium ... van Loon et al. (1999) new MSX sample. Superwind mass-loss rates ...

Jacco van Loon. Keele University. Dust wind structure. Radiative equilibrium ... van Loon et al. (1999) new MSX sample. Superwind mass-loss rates ...

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Stars - Stars Giants, Supergiants, Dwarfs . How we can tell a lot about stars from starlight. (You need a lot of physics)

Stars Giants, Supergiants, Dwarfs . How we can tell a lot about stars from starlight. (You need a lot of physics)

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Chapter 13: The Deaths of Stars PowerPoint PPT Presentation

Chapter 13: The Deaths of Stars - Chapter 13: The Deaths of Stars The Helix Nebula Planetary Nebulae From Supergiants to White Dwarfs Structure of an Old Low-Mass Star Structure of an Old High-Mass ...

Chapter 13: The Deaths of Stars The Helix Nebula Planetary Nebulae From Supergiants to White Dwarfs Structure of an Old Low-Mass Star Structure of an Old High-Mass ...

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Sun and Seasons PowerPoint PPT Presentation

Sun and Seasons - Stars range from very bright (supergiants) to very dim (dwarfs) ... Our Sun is a medium-bright dwarf. So is our Sun an average star? ...

Stars range from very bright (supergiants) to very dim (dwarfs) ... Our Sun is a medium-bright dwarf. So is our Sun an average star? ...

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H-R Diagrams PowerPoint PPT Presentation

H-R Diagrams - H-R Diagrams. Four Star Types. main sequence. giant. supergiant. white dwarf ... Which is brighter? the sun is hotter than a supergiant. supergiants are brighter ...

H-R Diagrams. Four Star Types. main sequence. giant. supergiant. white dwarf ... Which is brighter? the sun is hotter than a supergiant. supergiants are brighter ...

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Be Stars: Lessons from LongTerm Multitechnique Observations PowerPoint PPT Presentation

Be Stars: Lessons from LongTerm Multitechnique Observations - BA-supergiants - Nancy Morrison. Cosmic dust - Adolf Witt. Interstellar ... Solar system - Phil James (Chair) Outline. Brief history of studies of Be stars ...

BA-supergiants - Nancy Morrison. Cosmic dust - Adolf Witt. Interstellar ... Solar system - Phil James (Chair) Outline. Brief history of studies of Be stars ...

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Life Cycle of Stars PowerPoint PPT Presentation

Life Cycle of Stars - 8. Supergiants will explode into a supernova. ... When a massive star exploded producing a tremendous flash of light. This is called a supernova. ...

8. Supergiants will explode into a supernova. ... When a massive star exploded producing a tremendous flash of light. This is called a supernova. ...

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Winds of Massive Stars PowerPoint PPT Presentation

Winds of Massive Stars - Carrie Trundle. Tartu Aug. 2005. Tartu Aug. 2005 ... Trundle et al. 2004,2005 Blanketed SMC. Crowther et al. 2005 Blanketed Galactic ...

Carrie Trundle. Tartu Aug. 2005. Tartu Aug. 2005 ... Trundle et al. 2004,2005 Blanketed SMC. Crowther et al. 2005 Blanketed Galactic ...

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TYPES OF STARS PowerPoint PPT Presentation

TYPES OF STARS - TYPES OF STARS. By Sophie Werner and Billy Sheehan. Contents... Introduction. The 7 Types of Stars ... This show will tell you all you need to know about ...

TYPES OF STARS. By Sophie Werner and Billy Sheehan. Contents... Introduction. The 7 Types of Stars ... This show will tell you all you need to know about ...

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The Family of Stars PowerPoint PPT Presentation

The Family of Stars - 0 Chapter 9 The Family of Stars

0 Chapter 9 The Family of Stars

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Life Cycles of Stars PowerPoint PPT Presentation

Life Cycles of Stars - Life Cycles of Stars Stars Stars are a large hot balls of plasma that shine The Sun is the Star in our solar system A group of stars that form a recognizable shape ...

Life Cycles of Stars Stars Stars are a large hot balls of plasma that shine The Sun is the Star in our solar system A group of stars that form a recognizable shape ...

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Spectroscopy PowerPoint PPT Presentation

Spectroscopy - Spectroscopy the study of the colors of light (the spectrum) given off by luminous objects. Stars have absorption lines at different wavelengths where the energy ...

Spectroscopy the study of the colors of light (the spectrum) given off by luminous objects. Stars have absorption lines at different wavelengths where the energy ...

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Stars - ... the diameter and volume can be estimated The mass of the star can be estimated ... Light emitted from stars is analyzed using a spectrograph Absorption ...

... the diameter and volume can be estimated The mass of the star can be estimated ... Light emitted from stars is analyzed using a spectrograph Absorption ...

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Life Cycle of a Star PowerPoint PPT Presentation

Life Cycle of a Star - Creates the intense energy found in stars. Four types of stars make up the life of a star ... relationship between a star's surface temperature and absolute ...

Creates the intense energy found in stars. Four types of stars make up the life of a star ... relationship between a star's surface temperature and absolute ...

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THE LIFE CYCLE OF STARS PowerPoint PPT Presentation

THE LIFE CYCLE OF STARS - THE LIFE CYCLE OF STARS This star has entered the last stage of its life cycle The first stage of star formation is NUCLEAR FUSION Gravity pulls clouds ofgas and dust ...

THE LIFE CYCLE OF STARS This star has entered the last stage of its life cycle The first stage of star formation is NUCLEAR FUSION Gravity pulls clouds ofgas and dust ...

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Good Afternoon! PowerPoint PPT Presentation

Good Afternoon! - Good Afternoon! Please get your eInstruction remote and notebook.

Good Afternoon! Please get your eInstruction remote and notebook.

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Astronomy%20101%20The%20Solar%20System%20Tuesday,%20Thursday%20%20Tom%20Burbine%20tomburbine@astro.umass.edu PowerPoint PPT Presentation

Astronomy%20101%20The%20Solar%20System%20Tuesday,%20Thursday%20%20Tom%20Burbine%20tomburbine@astro.umass.edu - Title: Linking Asteroids and Meteorites through Reflectance Spectroscopy Author: Smithsonian Institution Last modified by: Tom Created Date: 5/23/2001 8:09:58 PM

Title: Linking Asteroids and Meteorites through Reflectance Spectroscopy Author: Smithsonian Institution Last modified by: Tom Created Date: 5/23/2001 8:09:58 PM

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ALMA Workshop UMD PowerPoint PPT Presentation

ALMA Workshop UMD - map. ALMA Workshop UMD. Margaret Meixner (STScI) 14 May 2004. The Sun: Quiet component: ... ALMA Workshop UMD. Margaret Meixner (STScI) 14 May 2004. NGC 7027 ...

map. ALMA Workshop UMD. Margaret Meixner (STScI) 14 May 2004. The Sun: Quiet component: ... ALMA Workshop UMD. Margaret Meixner (STScI) 14 May 2004. NGC 7027 ...

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A%20Survey%20of%20Local%20Group%20Galaxies%20Currently%20Forming%20Stars PowerPoint PPT Presentation

A%20Survey%20of%20Local%20Group%20Galaxies%20Currently%20Forming%20Stars - A Survey of Local Group Galaxies Currently Forming Stars

A Survey of Local Group Galaxies Currently Forming Stars

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Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode (presentation mode). - Betelgeuse Rigel 244 pc 152 pc d -6.8 -5.5 MV 0.14 0.41 mV Rigel Betelgeuse Back to our example of Betelgeuse and Rigel: Difference in absolute magnitudes: ...

Betelgeuse Rigel 244 pc 152 pc d -6.8 -5.5 MV 0.14 0.41 mV Rigel Betelgeuse Back to our example of Betelgeuse and Rigel: Difference in absolute magnitudes: ...

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Evolution of Massive Stars PowerPoint PPT Presentation

Evolution of Massive Stars - Luminous Blue Variables. h Car. 100 x. more luminous. in the MIR. Wolf Rayet Stars. Luminous Blue Variables. WNL. N,He,H. WNE. N,He. WC. C, O. H (& He) Burning ...

Luminous Blue Variables. h Car. 100 x. more luminous. in the MIR. Wolf Rayet Stars. Luminous Blue Variables. WNL. N,He,H. WNE. N,He. WC. C, O. H (& He) Burning ...

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Creation Astronomy PowerPoint PPT Presentation

Creation Astronomy - Saturn. Uranus. Neptune. Pluto. Our Moon. largest moon in the solar system ... the numbers show that moon would have been too close just one billion years ago ...

Saturn. Uranus. Neptune. Pluto. Our Moon. largest moon in the solar system ... the numbers show that moon would have been too close just one billion years ago ...

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Luminosity (relative to Sun) PowerPoint PPT Presentation

Luminosity (relative to Sun) - Rigel. Betelgeuse. Deneb. Arcturus. ... The bright star Betelgeuse is even more luminous than Aldebaran, but has a cooler surface. This makes it a red supergiant.

Rigel. Betelgeuse. Deneb. Arcturus. ... The bright star Betelgeuse is even more luminous than Aldebaran, but has a cooler surface. This makes it a red supergiant.

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Lives of Stars PowerPoint PPT Presentation

Lives of Stars - Lives of Stars Section 21.3 Life Cycle of Stars Nebula large cloud of gas and dust spread out in an immense volume Life Cycle of Stars Gravity pulls gas and dust ...

Lives of Stars Section 21.3 Life Cycle of Stars Nebula large cloud of gas and dust spread out in an immense volume Life Cycle of Stars Gravity pulls gas and dust ...

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Lives of Stars - Lives of Stars Section 21.3 Stephen Hawking - The Birth of Stars - YouTube Life Cycle of Stars Nebula large cloud of gas and dust spread out in an immense volume ...

Lives of Stars Section 21.3 Stephen Hawking - The Birth of Stars - YouTube Life Cycle of Stars Nebula large cloud of gas and dust spread out in an immense volume ...

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A Survey of Local Group Galaxies Currently Forming Stars PowerPoint PPT Presentation

A Survey of Local Group Galaxies Currently Forming Stars - M33 (3 fields) Phoenix. IC 10 IC 1613. NGC 6822 Sextans A. WLM Sextans B. How Are We Doing? ... Phoenix. WLM. What's Next? Spectroscopy! M31. N206 in M31. ob78 ...

M33 (3 fields) Phoenix. IC 10 IC 1613. NGC 6822 Sextans A. WLM Sextans B. How Are We Doing? ... Phoenix. WLM. What's Next? Spectroscopy! M31. N206 in M31. ob78 ...

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Good Afternoon! - ... Nova The explosion of a dying giant or supergiant star Kepler s Supernova Remnant http://hubblesite.org/gallery/album/query/supernova/ Super Giants ...

... Nova The explosion of a dying giant or supergiant star Kepler s Supernova Remnant http://hubblesite.org/gallery/album/query/supernova/ Super Giants ...

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Everything%20you%20always%20wanted%20to%20know%20about%20stars PowerPoint PPT Presentation

Everything%20you%20always%20wanted%20to%20know%20about%20stars - Everything you always wanted to know about stars

Everything you always wanted to know about stars

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Questions about Jao et al. 2005 - Questions about Jao et al' 2005

Questions about Jao et al' 2005

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Classification of Stars PowerPoint PPT Presentation

Classification of Stars - Plots surface temps of stars against their absolute magnitudes. ... Leftovers from a supernova that are so big as they contract, a hole is left in space. ...

Plots surface temps of stars against their absolute magnitudes. ... Leftovers from a supernova that are so big as they contract, a hole is left in space. ...

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Numerical Model Atmospheres (Hubeny PowerPoint PPT Presentation

Numerical Model Atmospheres (Hubeny - Based primarily upon temperature and electron density. Given abundances, ne, T we can find ... Column Density. Rewrite H.E. using column mass inwards (measured ...

Based primarily upon temperature and electron density. Given abundances, ne, T we can find ... Column Density. Rewrite H.E. using column mass inwards (measured ...

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X-ray Emission from Massive Stars: Using Emission Line Profiles to Constrain Wind Kinematics, Geometry, and Opacity PowerPoint PPT Presentation

X-ray Emission from Massive Stars: Using Emission Line Profiles to Constrain Wind Kinematics, Geometry, and Opacity - X-ray Emission from Massive Stars: Using Emission Line Profiles to Constrain Wind Kinematics, Geometry, and Opacity David Cohen Dept. of Physics and Astronomy

X-ray Emission from Massive Stars: Using Emission Line Profiles to Constrain Wind Kinematics, Geometry, and Opacity David Cohen Dept. of Physics and Astronomy

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Intensity and Distance PowerPoint PPT Presentation

Intensity and Distance - Intensity and Distance. Intensity depends. on luminosity and. distance. Inverse-square law ... Cameron Reed in 'The Composite Observational-Theoretical HR Diagram' ...

Intensity and Distance. Intensity depends. on luminosity and. distance. Inverse-square law ... Cameron Reed in 'The Composite Observational-Theoretical HR Diagram' ...

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Sulfur, manganese PowerPoint PPT Presentation

Sulfur, manganese - Sulfur, manganese in the Galaxy Mishenina T.V., Gorbaneva T.I., Paramonova O.P., Basak N.Yu., Kovtyukh V.V., Korotin S.A., Chekhonadskih F. +

Sulfur, manganese in the Galaxy Mishenina T.V., Gorbaneva T.I., Paramonova O.P., Basak N.Yu., Kovtyukh V.V., Korotin S.A., Chekhonadskih F. +

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X-ray Emission from Massive Stars: Using Emission Line Profiles to Constrain Wind Kinematics, Geometry, and Opacity - X-ray Emission from Massive Stars: Using Emission Line Profiles to Constrain Wind Kinematics, Geometry, and Opacity David Cohen Dept. of Physics and Astronomy

X-ray Emission from Massive Stars: Using Emission Line Profiles to Constrain Wind Kinematics, Geometry, and Opacity David Cohen Dept. of Physics and Astronomy

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Spectral Classification PowerPoint PPT Presentation

Spectral Classification - Spectral Classification Oh Be A Fine Guy/Gal; Kiss Me * They have even weaker hydrogen lines than F but along with the ionized metals, they have neutral metals.

Spectral Classification Oh Be A Fine Guy/Gal; Kiss Me * They have even weaker hydrogen lines than F but along with the ionized metals, they have neutral metals.

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Chapter 17 Stars PowerPoint PPT Presentation

Chapter 17 Stars - Chapter 17 Stars Properties of Stars Classifying Stars Hertzsprung-Russel (H-R) Diagram

Chapter 17 Stars Properties of Stars Classifying Stars Hertzsprung-Russel (H-R) Diagram

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Motivation: - The only hydrogen lines in the visible wavelength range. ... Russell-Saunders Coupling. l1. l3. l2. s1. s2. s3. e1. e3. e2. L. S. J. Filled shells: L = S = J = 0 ...

The only hydrogen lines in the visible wavelength range. ... Russell-Saunders Coupling. l1. l3. l2. s1. s2. s3. e1. e3. e2. L. S. J. Filled shells: L = S = J = 0 ...

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????? 2002 - I PowerPoint PPT Presentation

????? 2002 - I - Elena Barsukova, Valentina Klochkova & Azamat Valeev, ... Brightening before outburst is seen. Photometric history of V4332 Sgr. II. V band light curve ...

Elena Barsukova, Valentina Klochkova & Azamat Valeev, ... Brightening before outburst is seen. Photometric history of V4332 Sgr. II. V band light curve ...

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Stars, Galaxies, and the Universe PowerPoint PPT Presentation

Stars, Galaxies, and the Universe - Preview Multiple Choice Short Response Reading Skills Interpreting Graphics Multiple Choice 1. What accounts for different stars being seen in the sky during ...

Preview Multiple Choice Short Response Reading Skills Interpreting Graphics Multiple Choice 1. What accounts for different stars being seen in the sky during ...

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POST-MAIN SEQUENCE EVOLUTION PowerPoint PPT Presentation

POST-MAIN SEQUENCE EVOLUTION - Print your name (1) 1) Complete, and explain the balancing of, the ... Sirius B is a bound companion to the nearby very bright star Sirius (A): M=1.1 M ...

Print your name (1) 1) Complete, and explain the balancing of, the ... Sirius B is a bound companion to the nearby very bright star Sirius (A): M=1.1 M ...

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Nucleosynthesis and stellar lifecycles PowerPoint PPT Presentation

Nucleosynthesis and stellar lifecycles - Famous Eagle. Nebula image. Cool dark clouds. are close to ... AGB (Asymptotic Giant Branch) These differ in position on H-R diagram and in. interior structure ...

Famous Eagle. Nebula image. Cool dark clouds. are close to ... AGB (Asymptotic Giant Branch) These differ in position on H-R diagram and in. interior structure ...

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Stars and Their Characteristics PowerPoint PPT Presentation

Stars and Their Characteristics - Is the big dipper the largest? No. Ursa Major (big bear) Circumpolar constellations ... Some like the big dipper only change the position in the sky ...

Is the big dipper the largest? No. Ursa Major (big bear) Circumpolar constellations ... Some like the big dipper only change the position in the sky ...

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Solid - Properties of Thermal ... PowerPoint Presentation PowerPoint Presentation PowerPoint Presentation PowerPoint Presentation Why do the properties of some stars ...

Properties of Thermal ... PowerPoint Presentation PowerPoint Presentation PowerPoint Presentation PowerPoint Presentation Why do the properties of some stars ...

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Stars - Direct: Heliocentric stellar parallaxes (AU as baseline) Smaller parallax, greater distance. Inverse relation: Distance is inversely proportional to parallax angle ...

Direct: Heliocentric stellar parallaxes (AU as baseline) Smaller parallax, greater distance. Inverse relation: Distance is inversely proportional to parallax angle ...

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Stellar Properties PowerPoint PPT Presentation

Stellar Properties - Advantages: relatively easy and good for fainter targets. Disadvantages: need good conditions ('photometric') for reliable measurements ...

Advantages: relatively easy and good for fainter targets. Disadvantages: need good conditions ('photometric') for reliable measurements ...

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Astronomy 192401 PowerPoint PPT Presentation

Astronomy 192401 - ... take out a sheet of paper and put your name and today's ... Absolute Magnitude the apparent magnitude a star would have if it were 10 pc ... mass of a star ...

... take out a sheet of paper and put your name and today's ... Absolute Magnitude the apparent magnitude a star would have if it were 10 pc ... mass of a star ...

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Fundamentals of Astronomy: - Fundamentals of Astronomy:

Fundamentals of Astronomy:

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SO Coaches Clinic 2002 - SO Coaches Clinic 2002

SO Coaches Clinic 2002

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Star Properties PowerPoint PPT Presentation

Star Properties - Twinkle twinkle little star, how I wonder what you are ... ... Star Properties

Twinkle twinkle little star, how I wonder what you are ... ... Star Properties

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A cosmic abundance standard PowerPoint PPT Presentation

A cosmic abundance standard - ... N, Mg, Al, Ne, Fe & others (Munich Observatory N. ... tailored. modelling. Similar results for He, N, O Ne, Mg, Si, Fe. So far O, Mg & Si confirmed by ...

... N, Mg, Al, Ne, Fe & others (Munich Observatory N. ... tailored. modelling. Similar results for He, N, O Ne, Mg, Si, Fe. So far O, Mg & Si confirmed by ...

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Magnetic Fields in the Envelopes of Late-Type Stars: Circular Polarization of H2O Masers PowerPoint PPT Presentation

Magnetic Fields in the Envelopes of Late-Type Stars: Circular Polarization of H2O Masers - 'Onion model' Dust at few AU. Molecules until. dissociation by UV. Excitation varies. SiO at few AU ... magnetic shaping of the outflow (Garc a-Segura, 1999) ...

'Onion model' Dust at few AU. Molecules until. dissociation by UV. Excitation varies. SiO at few AU ... magnetic shaping of the outflow (Garc a-Segura, 1999) ...

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The Universe PowerPoint PPT Presentation

The Universe - The Universe 8th Grade Science

The Universe 8th Grade Science

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Life cycle of a star - Life cycle of a star Birth of Stars All stars are born in nebulae, huge clouds of dust and gas These collapse under gravitational forces, forming protostars These ...

Life cycle of a star Birth of Stars All stars are born in nebulae, huge clouds of dust and gas These collapse under gravitational forces, forming protostars These ...

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Supergiants PowerPoint PPT Presentations