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Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake, Rowin Meijerink, Joan Najita, John Carr

Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

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Page 1: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Observations of Water and other molecules in Protoplanetary Disk

Atmospheres

Colette SalykUT Austin/McDonald ObservatoryKlaus Pontoppidan, Geoffrey Blake, Rowin Meijerink,

Joan Najita, John Carr

Page 2: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Water vapor and organics detected in ‘typical’ circumstellar disks with Spitzer-IRS

Spitzer IRS: Carr & Najita 2008; Salyk et al. 2008 T~500-1000 K

Page 3: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Ground-based follow-up confirms origin in planet-forming region of disk

Salyk et al. 2008

Line profiles consistent with ~few AU emitting radii

Page 4: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

What disk processes might water emission probe?

Radial transport of water via diffusion (out) and icy-body migration (in)

“snow line”

e.g. Stevenson & Lunine 1988; Ciesla & Cuzzi 2006

vapor freezes out

vapor diffuses outwards

low vapor pressurehigh vapor pressure

solids migrate inwardssolids evaporate

Page 5: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

What disk processes might water emission probe?

Radial transport of water via diffusion (out) and icy-body migration (in)

Water self-shielding

Bethell & Bergin 2009

Page 6: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

What disk processes might water emission probe?

Radial transport of water via diffusion (out) and icy-body migration (in)

Water self-shielding

Radiative processes

Condensation fronts and vertical transport

Disk chemistry

Small dust grain growth/settling

Clearly a challenge to disentangle multiple effects

Page 7: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

GO5 program: Water in Disks (PI: J. Carr)

-52 class II disks in multiple star-forming regions-Designed to cover a range of stellar/disk parameters

Page 8: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

GO5 program: Water in Disks (PI: J. Carr)

-52 class II disks in multiple star-forming regions-Designed to cover a range of stellar/disk parameters-Subset of these disks + archived programs results in sample shown here

Page 9: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Sampled disks show significant variety

Page 10: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Pontoppidan et al., in prep

Page 11: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Pontoppidan et al., in prep

-Lines are actually spectrally uresolved line blends at the resolution of Spitzer-IRS -Lines probe a large range of excitation temperatures

Page 12: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Water vapor and organic emission is commonaround low-mass young stars

Pontoppidan et al. , in prep

Page 13: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Detection rates drop precipitously for SpT<G

Pontoppidan et al. , in prep

Page 14: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Transitional disks do not show emission

Page 15: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

Emission of water correlates with CO emission

Page 16: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

LTE models can be used to estimate density, T

Page 17: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,

But in general do a poor job of matching the data

Page 18: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,
Page 19: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,
Page 20: Observations of Water and other molecules in Protoplanetary Disk Atmospheres Colette Salyk UT Austin/McDonald Observatory Klaus Pontoppidan, Geoffrey Blake,