Optical characterization of a new young stellar population in the serpens molecular cloud

Astrophysical Journal

Volumn 691, Issue 1, 2009, Pages 672-686

  Oliveira, Isa ^a,b   Merín, Bruno ^b,c   Pontoppidan, Klaus M ^a   Van Dishoeck, Ewine F ^b,d   Overzier, Roderik A ^e   Hernández, Jesús ^f,g   Sicilia Aguilar, Aurora ^h   Eiroa, Carlos ⁱ   Montesinos, Benjamin ^j,k  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b LEIDEN UNIVERSITY   (Netherlands)

^c Research and Scientific Support Department   (Netherlands)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^e MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^f UNIVERSITY OF MICHIGAN   (United States)

^g CENTRO DE INVESTIGACIONES DE ASTRONOMÍA   (Venezuela)

^h MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

ⁱ UNIVERSIDAD AUTÓNOMA DE MADRID   (Spain)

^j INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^k EUROPEAN SPACE AGENCY   (Spain)

more..

Author keywords

Hertzsprung Russell diagram; ISM: individual (Serpens); planetary systems: protoplanetary disks; stars: pre main sequence

Indexed keywords

EID: 67650579539     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/691/1/672     Document Type: Article

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