Three intermediate-mass young stellar objects with different properties emerging from the same natal cloud in IRAS 00117+6412

Astronomy and Astrophysics

Volumn 510, Issue 1, 2010, Pages

  Palau, Aina ^a   Sanchez Monge A ^b   Busquet, G ^b   Estalella, R ^b   Zhang, Q ^c   Ho, P T P ^c,d   Beltran M T ^e   Beuther, H ^f  

^a CENTRO DE ASTROBIOLOGÍA CSIC INTA   (Spain)

^b UNIVERSITY OF BARCELONA   (Spain)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^e INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Dust, extinction; Ion(h)(ii) regions; ISM: individual objects: IRAS 00117+6412; Radio continuum: ISM; Stars: formation

Indexed keywords

ASSOCIATED WATER; COLUMN DENSITY; DENSE GAS; DUST EMISSION; DUST, EXTINCTION; EASTERN EDGE; HIGH VELOCITY; I-PHASE; INITIAL CONDITIONS; ISM: INDIVIDUAL OBJECTS; MASS STARS; MILLIMETER SOURCES; NEAR INFRARED; NEAR-INFRARED EMISSIONS; PROTOSTARS; RADIO CONTINUUM: ISM; SHELL-LIKE STRUCTURES; STAR FORMATIONS; STAR-FORMATION PROCESS; VELOCITY GRADIENTS; WATER MASERS; YOUNG STELLAR OBJECTS;

DUST; INFRARED DEVICES; IONS; MASERS; STARS; ULTRASONICS;

LEAKAGE (FLUID);

EID: 77149169717     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913215     Document Type: Article

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