Sitko Synoptic Disksirtfweb.ifa.hawaii.edu/meetings/irtf_future_2018/... · 2018. 3. 2. · Return...
Transcript of Sitko Synoptic Disksirtfweb.ifa.hawaii.edu/meetings/irtf_future_2018/... · 2018. 3. 2. · Return...
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Synoptic Observations of Young Starswith Planet-Building Disks
IRTF Workshop 2018
Mike Sitko (U Cincinnati & Space Sci. Inst.) Monika Pikhartova (U Cincinnati)
Carol Grady (Eureka Scientific, Inc.) John Wisniewski (U Oklahoma)
Evan Rich (U Oklahoma)
SCHEDULING!
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DIAGNOSTICS - gas & DUST
IRTF Workshop 2018
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2003 - inner rim was 20% bigger!
– 11 –
-0.4 -0.2 0.0 0.2 0.4AU
-0.4
-0.2
0.0
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’Standard’ inner-rim model (K band image)
0.07
0.11
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(Sur
face
Brig
htne
ss (e
rg/s
/cm
^2) )
^0.1
-0.6 -0.4 -0.2 0.0 0.2 0.4 0.6AU
-0.6
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’Standard’ inner-rim + gas model (K band image)
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(Sur
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ss (e
rg/s
/cm
^2) )
^0.1
Fig. 1.— Representative models for near-IR emission in Herbig Ae stars. a) Left panel. A
standard curved dust-rim-only model (Isella & Natta 2005; Tannirkulam et al. 2007) wherethe dust sublimation temperature is a power-law function of gas density (Pollack et al. 1994).b) Right panel. Gas emission (modeled as a uniform disk centered on the star) has been
added inside the dust rim in order to smooth out the emission profile.
resolved inner gas
Adapted (and embellished) from Tannirkulam et al. 208, ApJ, 677, L51
IRTF Workshop 2018
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Wisniewski et al.2008, ApJ, 682, 548
IRTF Workshop 2018
HD 163296 = MWC 275
Increased disk wall height - increased near IR flux - causes increased shadowing and drop in mid-IR flux ("see-saw")
LRLL 31 - Muzerolle et al. 2009
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Ellerbroek et al. 2014, A&A, 563, A87
IRTF Workshop 2018
IR only sparsely sampled
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IRTF Workshop 2018
Periodic HH Knots ~16 year photometric periodProper motion traceback
HD 163296 = MWC 275
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Ellerbroek et al. 2014, A&A, 563, A87
IRTF Workshop 2018
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jet thermal emission
middle disk no longer shadowedV band drop
from Monika Pikhartova et al. AAS 2017 & 2018
MCRT Model
jet blocks direct illumination by star
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IRTF Workshop 2018
What Next?Coordinate with Interferometers (again)Already did this with Keck (no longer KI) & VLTI/MATISSE (mid-IR 4T)Discussed with CHARA Director and 6T Scientists Monnier last year
Kraus et al. 2013
Millan-Gabet et al. 2016
MWC 480 CHARA 6T
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IRTF Workshop 2018
What Next?Support of JWST (& other Coronagraphs) - What IS the illumination of thedisks? (bright stars observable with JWST/MIRI coronagraph, NIRISS-SAM)
SAO 206462(Muto et al. 2012)
MWC 480 (Kusakabe et al. 2012)
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IRTF Workshop 2018
What Next?
Return of MIRSI with Visible-Wavelength (Guider) Capability and Extension to mid-IR - variability, including “see-saw” behavior, daytime observing
SpeX
MIRSI
?