Near-infrared spectroscopy of young stellar objects

1994 ◽  
Vol 425 ◽  
pp. 231 ◽  
Author(s):  
D. M. Kelly ◽  
G. H. Rieke ◽  
B. Campbell
Keyword(s):  
Infrared Spectroscopy ◽  
Near Infrared Spectroscopy ◽  
Near Infrared ◽  
Young Stellar Objects ◽  
Stellar Objects

scholarly journals AKARI Near-Infrared Spectroscopy: Detection of H 2 O and CO 2 Ices toward Young Stellar Objects in the Large Magellanic Cloud

2008 ◽  
Vol 686 (2) ◽  
pp. L99-L102 ◽  
Author(s):  
Takashi Shimonishi ◽  
Takashi Onaka ◽  
Daisuke Kato ◽  
Itsuki Sakon ◽  
Yoshifusa Ita ◽  
...  
Keyword(s):  
Infrared Spectroscopy ◽  
Near Infrared Spectroscopy ◽  
Near Infrared ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Young Stellar Objects ◽  
Stellar Objects

scholarly journals Medium-resolution near-infrared spectroscopy of massive young stellar objects

2017 ◽  
Vol 472 (3) ◽  
pp. 3624-3636 ◽  
Author(s):  
R. Pomohaci ◽  
R. D. Oudmaijer ◽  
S. L. Lumsden ◽  
M. G. Hoare ◽  
I. Mendigutía
Keyword(s):  
Infrared Spectroscopy ◽  
Near Infrared Spectroscopy ◽  
Near Infrared ◽  
Young Stellar Objects ◽  
Stellar Objects ◽  
Medium Resolution

scholarly journals The stellar content of obscured Galactic giant H II regions

2003 ◽  
Vol 212 ◽  
pp. 458-466
Author(s):  
Robert D. Blum
Keyword(s):  
Infrared Spectroscopy ◽  
Near Infrared Spectroscopy ◽  
Near Infrared ◽  
Star Clusters ◽  
Stellar Populations ◽  
Radio Continuum ◽  
Young Stellar Objects ◽  
Great Promise ◽  
High Angular Resolution ◽  
Stellar Content

Current research using near-infrared techniques for investigating stellar populations in massive Galactic star clusters is reviewed. In particular, I discuss in some detail a survey of obscured Galactic Giant H ii (GH ii) regions and the associated stellar clusters embedded in them. The regions have been selected as the most luminous radio continuum sources. This selection criteria has the consequence that the observed clusters are among the youngest massive star clusters in the Galaxy. The emergent stellar populations are further studied through near-infrared spectroscopy of the brighter members, a number of which are young stellar objects with signatures of dense circumstellar material which might arise from in or out-flows, or in disks. New results from 8m class telescopes employing velocity resolved near-infrared spectroscopy and high angular resolution mid-infrared imaging hold great promise for future detailed investigations.

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