A Mid-Infrared Study of Dust Evolution: Protoplanetary Disks, Circumstellar Envelopes, and Lmircam Development

2011 ◽  
Author(s):  
Jarron Michael Leisenring
Keyword(s):  
Protoplanetary Disks ◽  
Circumstellar Envelopes ◽  
Infrared Study ◽  
Mid Infrared ◽  
Dust Evolution

scholarly journals A mid-infrared study of very low mass stars and brown dwarfs in Upper Scorpius

2006 ◽  
Vol 463 (2) ◽  
pp. 641-646 ◽  
Author(s):  
H. Bouy ◽  
N. Huélamo ◽  
E. L. Martín ◽  
D. Barrado y Navascués ◽  
M. Sterzik ◽  
...  
Keyword(s):  
Brown Dwarfs ◽  
Low Mass Stars ◽  
Infrared Study ◽  
Mid Infrared ◽  
Low Mass

scholarly journals Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet

2019 ◽  
Vol 885 (1) ◽  
pp. 91 ◽  
Author(s):  
Joanna Dra̧żkowska ◽  
Shengtai Li ◽  
Til Birnstiel ◽  
Sebastian M. Stammler ◽  
Hui Li
Keyword(s):  
Protoplanetary Disks ◽  
Hydrodynamic Models ◽  
Dust Evolution

scholarly journals Dust Evolution in Protoplanetary Disks

2018 ◽  
pp. 1-16
Author(s):  
Sean M. Andrews ◽  
Tilman Birnstiel
Keyword(s):  
Protoplanetary Disks ◽  
Dust Evolution

Further mid-infrared study of the rho Ophiuchi cloud young stellar population: Luminosities and masses of pre-main-sequence stars

1994 ◽  
Vol 434 ◽  
pp. 614 ◽  
Author(s):  
Thomas P. Greene ◽  
Bruce A. Wilking ◽  
Philippe Andre ◽  
Erick T. Young ◽  
Charles J. Lada
Keyword(s):  
Stellar Population ◽  
Main Sequence ◽  
Main Sequence Stars ◽  
Infrared Study ◽  
Mid Infrared ◽  
Rho Ophiuchi

scholarly journals Mass-losing AGB Stars in the LMC

2000 ◽  
Vol 177 ◽  
pp. 145-151
Author(s):  
Jacco Th. Van Loon ◽  
Albert A. Zijlstra ◽  
Patricia A. Whitelock ◽  
Cecile Loup ◽  
L.B.F.M. Waters
Keyword(s):  
Mass Loss ◽  
Optical Depth ◽  
Agb Stars ◽  
Circumstellar Envelopes ◽  
Carbon Stars ◽  
Infrared Study ◽  
Tentative Evidence ◽  
Loss Rates

We show the results of an infrared study of a sample of heavily obscured AGB stars in the LMC. Both carbon-rich and oxygen-rich mass-losing AGB stars can be found at both high and low luminosities, but the percentage of carbon stars decreases with increasing luminosity. The optical depth of the circumstellar envelopes also decreases with increasing luminosity, while the mass-loss rates are (nearly) constant with luminosity. We also show tentative evidence for having found the first post-AGB stars in the LMC.

Mid-infrared study of the molecular structure variability of insoluble organic matter from primitive chondrites

Icarus ◽  
2013 ◽  
Vol 223 (1) ◽  
pp. 534-543 ◽  
Author(s):  
F.-R. Orthous-Daunay ◽  
E. Quirico ◽  
P. Beck ◽  
O. Brissaud ◽  
E. Dartois ◽  
...  
Keyword(s):  
Molecular Structure ◽  
Organic Matter ◽  
Infrared Study ◽  
Mid Infrared ◽  
Insoluble Organic Matter

scholarly journals Mid-infrared study of stones from the Sutter's Mill meteorite

2014 ◽  
Vol 49 (11) ◽  
pp. 2017-2026 ◽  
Author(s):  
Michel Nuevo ◽  
Scott A. Sandford ◽  
George J. Flynn ◽  
Susan Wirick
Keyword(s):  
Infrared Study ◽  
Mid Infrared
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