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YSOs: Young Stellar Objects

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... but are warmed by that visible light and so radiate in the IR visible light image IR light image mosaic IR stars in Orion IR star DC303.8-14.2 visible light ... – PowerPoint PPT presentation

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Title: YSOs: Young Stellar Objects


1
YSOs Young Stellar Objects
Provide evidence for planet-forming nebular disks
around stars
Dusty cocoon surrounding YSO
2
Different types of YSOs 1) IR stars 2)
Proplyds 3) Herbig-Haro objects 4) T-Tauri
stars 5) Beta Pictoris systems Range from
protostars to newly-formed stars
3
  • IR stars
  • infrared protostars
  • show excess emission in IR compared to visible
    wavelengths
  • explained by dust cocoons surrounding protostar
  • these cocoons obscure the visible light from the
    central star-like object, but are warmed by that
    visible light and so radiate in the IR

4
IR stars in Orion
visible light image
IR light image mosaic
5
IR star DC303.8-14.2
visible light (700 nm), showing dust
IR light (1.65 um), showing ring of warmed dust
around embedded IR star
IR light (2.17 um), showing inner clumps (shocked
gas?)
6
  • Proplyds protoplanetary disks
  • dusty cocoons seen around YSOs
  • first seen clearly in the Orion Nebula

7
Proplyd with evidence for infalling matter
(nebular disk shocks)
Disk 800 AU across
Pattern of methanol emission can be explained by
clumpy accretion onto surface of disk
8
  • Herbig-Haro
  • Objects
  • YSOs with
  • disks bipolar
  • outflows

9
Bipolar jet
10
  • T-Tauri star
  • catchall term for many types of YSOs
  • YSO has not yet ignited H it follows Hayashi
    track in luminosity temperature
  • YSO can show evidence for rapid rotation, strong
    magnetic field, strong stellar winds, short-lived
    brightness spikes (FU-Orionis outbursts), excess
    IR emission

H-R diagram showing Hayashi track (4-7) and Main
Sequence trend (grey band)
http//www.go.ednet.ns.ca/larry/stars/prtostar.ht
ml
11
  • Beta Pictoris-type system
  • newly-formed star that still has a surrounding
    dust disk
  • YSO has achieved H to He fusion and falls on
    Main
  • Sequence trend
  • dust disk soon to be destroyed, either by
  • stellar winds (material blown out of system)
  • or
  • movement to star (e.g., via Poynting-Robertson
    effect)

12
Dust disk around Beta Pictoris seen edge on
colors represent light intensities
waves in disk probably
caused by interaction with planets
13
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