The youngest massive protostars in the Large Magellanic Cloud

Astronomy and Astrophysics

Volumn 518, Issue 7-8, 2010, Pages

  Sewilo M ^a   Indebetouw, R ^b   Carlson, L R ^c   Whitney, B A ^d   Chen, C H R ^b   Meixner, M ^a,e   Robitaille, T ^e   Van Loon, J Th ^f   Oliveira, J M ^f   Churchwell, E ^g   Simon, J D ^h   Hony, S ⁱ   Panuzzo, P ⁱ   Sauvage, M ⁱ   Roman Duval, J ^a   Gordon, K ^a   Engelbracht, C ^j   Misselt, K ^j   Okumura, K ⁱ   Beck, T ^a   Hora, J ^e   Woods, P M ^k   more..

^a STScI   (United States)

^b UNIVERSITY OF VIRGINIA   (United States)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d Center for Extrasolar Planetary Systems   (United States)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f KEELE UNIVERSITY   (United Kingdom)

^g UNIVERSITY OF WISCONSIN MADISON   (United States)

^h CARNEGIE OBSERVATORIES   (United States)

ⁱ CEA SACLAY   (France)

^j UNIVERSITY OF ARIZONA   (United States)

^k UNIVERSITY OF MANCHESTER   (United Kingdom)

more..

Author keywords

Magellanic Clouds; Stars: formation; Stars: protostars

Indexed keywords

ACCRETION RATE; COMPACT SOURCES; DEMONSTRATION PROGRAMS; EVOLUTIONARY STAGE; FAR-INFRARED; HERSCHEL; LARGE MAGELLANIC CLOUDS; LONG WAVES; MAGELLANIC CLOUDS; PROTOSTARS; RADIATIVE TRANSFER MODEL; SPECTRAL ENERGY DISTRIBUTION; SPITZER; STARS: FORMATION; STARS: PROTOSTARS; YOUNG STELLAR OBJECTS;

CLOUDS; GALAXIES; MODELS; PHYSICAL PROPERTIES; PLASMA WAVES; RADIATIVE TRANSFER; SPECTROSCOPY;

STARS;

EID: 77957764881     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014688     Document Type: Article

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