Title: YSOs: Young Stellar Objects
1YSOs Young Stellar Objects
Provide evidence for planet-forming nebular disks
around stars
Dusty cocoon surrounding YSO
2Different 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
4IR stars in Orion
visible light image
IR light image mosaic
5IR 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
7Proplyd 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
9Bipolar 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
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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)
12Dust disk around Beta Pictoris seen edge on
colors represent light intensities
waves in disk probably
caused by interaction with planets
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