The young stellar population in the Serpens Cloud Core: An ISOCAM survey

Astronomy and Astrophysics

Volumn 421, Issue 2, 2004, Pages 623-642

  Kaas, A A ^a,b   Olofsson, G ^b   Bontemps, S ^b,c   Andre P ^d   Nordh, L ^b   Huldtgren, M ^b   Prusti, T ^e   Persi, P ^f   Delgado, A J ^g   Motte, F ^d   Abergel, A ^h   Boulanger, F ^h   Burgdorf, M ⁿ   Casali, M M ⁱ   Cesarsky, C J ^d   Davies, J ^j   Falgarone, E ^k   Montmerle, T ^l   Perault, M ^k   Puget, J L ^h   Sibille, F ^m   more..

^a NORDIC OPTICAL TELESCOPE   (Spain)

^b STOCKHOLM OBSERVATORY   (Sweden)

^c OBSERVATOIRE DE BORDEAUX   (France)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e Department of ESA   (Netherlands)

^f CNR   (Italy)

^g INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^h UNIVERSITÉ PARIS SUD   (France)

ⁱ UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^j UNIVERSITY OF HAWAII   (United States)

^k ECOLE NORMALE SUPÉRIEURE   (France)

^l LABORATOIRE D ASTROPHYSIQUE   (France)

^m OBSERVATOIRE DE LYON   (France)

ⁿ CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

ISM: individual objects: Serpens Cloud Core; Stars: formation; Stars: low mass, brown dwarfs; Stars: luminosity function, mass function; Stars: pre main sequence

Indexed keywords

BROWN DWARFS-ISM; INDIVIDUAL OBJECTS; LUMINOSITY FUNCTION; MASS FUNCTION-STARS; PRE-MAIN-SEQUENCE; SERPENS CLOUD CORE; STARS;

COLOR; CONDENSATION; DATA ACQUISITION; DEMODULATION; INFRARED RADIATION; MAPPING; PHOTOMETRY; SPECTRUM ANALYSIS; STATISTICAL METHODS;

CLOUDS;

EID: 3042760556     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035775     Document Type: Review

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