Agbs PowerPoint PPT Presentations

C and s-elements are formed in TP-AGB stars ... MISTERY! Promising solution: formation of barium stars in binary systems (McClure et al. 1980) ...

AGB stars and the two sources of neutrons ... A few Halo CEMP-s dwarf stars with no dilution [hs/ls] vs [s/Fe] Extrinsic AGBs ...

CSI Challenge #10 Word Scramble Week 10 - Monday Word Scramble 1. FMAIYINGGN SLAGS 2. KIN DPA 3. ERAPP ADP 4. RETZESEW 5. ESABELLA AGBS Magnifying Glass Ink Pad Paper ...

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S-process nucleosynthesis in AGB stars at solar metallicity. ... ls(Sr, Y, Zr) hs(Ba, La, Cs, Nd,Sm) Pb. 9. IRAS 0713 1005. 10. Extrinsic AGBs. 2. 1. 1. 2 ...

Workshop on Renewable Energy and Poverty Reduction in Africa: ... Telephone: 33 (01) 44 37 30 03. Email: lagbemabiese@unep.fr. Blog: http://agbe.typepad.com ...

Barium Stars Theoretical interpretation. Laura Husti. 2. Extrinsic AGBs. 2. 1. 1. 2. 2. 2 ... theoretical fits for the element abundances degeneracy in AGB ...

The first array dedicated to VLBI astrometry. New technique : ... PL relation of Mira (Feast et al 1989) PL relation for AGBs (Wood 2000) High Energy Objects ...

(1) Dipartimento di Fisica Generale , Universit di Torino, 10125 Torino ( Italy) ... interstellar medium before the solar system formed. ...

The MonKey Project An Update on Stellar Yields

Supervisor: Anja C. Andersen. Dust in Young Galaxies. 2. The code. Radiative transfer ... Dust Extinction in Starburst Galaxies at z = 3 6. Dust Creation in ...

... statistic (Drasco et al. 2003), Probability Event Horizon (Coward et al. 2005) ... Neutron star formation: Blair & Ju 1996, Coward et al. 2001-02, Howell et al. ...

Transient torus A unified after-AGB binary scenario? Frankowski Institut d Astronomie et d Astrophysique, ULB, Brussels, Belgium The family of after AGB ...

First examples of feasible science of interest for THIS meeting ... stars black-bodies (Rayleigh-Jeans, l-4) ... objects: brown dwarfs, giant planets, ...

STRATEGIC OBJECTIVES IN FRONT-END SYSTEMS ... Front-end systems play a key role in closing informational asymmetries ... Most industrial end-users, natural gas ...

501 isotopes 701 isotopes. 700 reactions 1200 reactions. Gl04: Gallinium 2004 ... Neutron cross sections of unstable isotopes far from the stability valley. ...

Lebzelter & Hron, 2003, A&A 411, 533 542 'Technetium and the third ... Echelle Spectrograph. Last instrument of the. first generation. Basic characteristics: ...

Instituto de Astrof sica de Canarias, Seminar presentation of IAC postdocs, ... HdC stars and some RCBs are strongly enriched in 18O (16O/18O~0.2 4) but C and N ...

[ls/Fe] versus [Fe/H] ls = Y, Zr M = 1.3 MT. M = 1.5 MT. M = 2 MT. M = 3 MT. 3. 2. 1. 3 ... To reproduce stars with both s r enhancements ...

The Origin of the Elements Heavier than Fe - 25th - 27th September. 2. Outline: ... Low Na, and low [ls/Fe] observed in main-sequence or turnoff stars as indicator ...

Institut d'Astronomie et d'Astrophysique, ULB, Brussels, Belgium. The family of 'after AGB' binaries. The ... e.g. Podsiadlowski, Joss & Hsu 1992, ApJ 391, 246 ...

Is the outer halo filled with tidal streams from disrupted dwarf galaxies that ... (Bullock et al. 2002, Font et al. 2001, 2005, Johnston et al. 2002, etc. ...

MAY 1- SPRING LECTURE DAY Clear off your desks- no writing required * * * * Key concepts to remember: Remember: Conceptual Accuracy- signing what is meant, not the ...

The huge pulse and H remixing at very low metallicities ... This implies a huge primary 22Ne neutron source at the end of core He-burning as ...

... the chemical composition of the dust grains (ISO, mm/submm, radio) ... ISO data in most cases; also from submm and/or radio observations) ... HD 183143. Pedro ...

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In collaboration with P. Garc a-Lario (IDC-ESAC), B. Plez (GRAAL, France), A. ... metallicity lower dust production (van Loon 00) less efficient mass loss longer ...

Some Best Practices for Airport Pavement Maintenance, Repairs and Rehabilitation: Methods and Materi

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 ...

some quotes from IAU Symposium 187 'can we avoid more data = less understanding ? ... funny binaries ? nucleosynthesis - effect of rate uncertainties ...

... ha) is defined in the study as a biomass of growing stock trees greater than 2.5 ... Topography: flat to rolling (elevation from 232 to 459 m) ...

SCIENTIFIC EVIDENCE TO SUPPORT SOME CULTURAL AND MAGICO-RELIGIOUS PRACTICES IN ... People with such clairvoyant ability abound elsewhere. ...

Key objects in the study of the dramatic morphological and chemical changes ... physical parameters of the stellar photosphere (log Teff, log g); from which ...

Title: PowerPoint-Pr sentation Author: Prof. Dr. Thomas Rauscher Last modified by: Prof Dr Thomas Rauscher Created Date: 1/4/2000 9:27:55 AM Document presentation format

The neutron burst required is a natural consequence of Type II supernova explosions ... from Type II, not Type Ia supernovae, as such a burst does not occur in SN Ia ...

Galactic latitude distribution. Statistical indicator of the mass of a population of stars. High ... Evolutionary status Galactic latitude statistics ...

Week 2 MCS101 MEDIA INSTITUTIONS Media Structures and Institutions brahim Cans zo lu, Burak Do u ibrahim.cansizoglu@ieu.edu.tr, burak.dogu@ieu.edu.tr

Chemical Signatures from Stars in the Nearby Dwarf Galaxies

C-enhanced low temperature opacities: why we need it ... Izzard et al. Karakas et al. FRANEC. 1.91e-7. Ba. M2 Z2m2. M2 Z2m2 (ETA=4) M2 Z2m2. M2 Z2m2 ...

Post-AGB stars Pedro Garc a-Lario European Space Astronomy Centre ESA,Villafranca del Castillo, Madrid Why post-AGB stars? Key objects in the study of the dramatic ...

Status of the project & next actions. First programmes: ... CAMISTIC, bolometer for 200 and 350 mm. Priority required by the community (even in this meeting) ...

Attended lecture course on a large range of topics including many in astrophysics. ... blue YMCs, for whom the blue photosphere of the young stars is directly visible ...

MAIN SEQUENCE STARS, Red Giants and White Dwarfs Stars are powered by fusion reactions. When a fuel is exhausted the star s structure changes dramatically, producing

High mass X ray binaries: O B star companion # Low mass X ray binaries: Low mass star, ~ 1 Mo ... s nuc; typically T 7 8 x 108 K) # At this temperatures ...

Why is the study of ... Trumpler (1930) found that distant stars dimmed by something ... YMCs, for whom the blue photosphere of the young stars is directly ...

Announcements Quiz 4 - March 4 Stellar evolution Low-mass stars Binaries High-mass stars Supernovae Synthesis of the elements WWW lab is available at the class WWW site

Global Aircraft Gearbox Market is estimated to reach $6.24 billion by 2025; growing at a CAGR of 8.2% from 2017 to 2025

In H II regions along spiral arms HII regions M51-HST * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * * The centre of the Crab ...

AGB Star Yields for Everyone John Lattanzio1 and Amanda Karakas2 1: Centre for Stellar and Planetary Astrophysics, Monash University,Australia 2: Origins Institute ...

Variable Stars in the Old Dwarf Spheroidal Galaxies, SDSS dSph s, and Globular Clusters Charles Kuehn Michigan State University

Learning outcome Knowledge of the observed P-L-relations for AGB stars Knowledge of the ... LMC P-L and amplitude Sequence E Sequence D LPVs in Clusters Linear ...

... fyldstf qmd klg tf]Sg ;Sb5g / k|fyldstf qmd ;f]xL bnsf] ;'rLdf l;ldt x'g] rng 5. ... fgf bnn] klg k|ltlglwTj ug]{ ePsf] x'Fbf bnsf] 6'lqmg] qmd a9g ;S5. ...

X-ray Photospheres Klaus Werner Institute for Astronomy and Astrophysics, University of T bingen, Germany

Stellar Fuel, Nuclear Energy and Elements How do stars shine? E = mc2 How did matter come into being? Big bang stellar nucleosynthesis How did different elements form?

... C O Ne Si H-He CNO CNO Ne Na Cycle NO ROTATION Main Sequence Convective Core Red Supergiant Pre SN II ROTATION Main Sequence ... 1029 AGB Stars: Pumo, D ...

Title: PowerPoint Presentation Author: NSCL Last modified by: schatz Created Date: 4/10/2003 2:25:26 AM Document presentation format: On-screen Show