A "starless'' core that isn't:: Detection of a source in the L1014 dense core with the Spitzer Space Telescope

被引:151
作者
Young, CH
Jorgensen, JK
Shirley, YL
Kauffmann, J
Huard, T
Lai, SP
Lee, CW
Crapsi, A
Bourke, TL
Dullemond, CP
Brooke, TY
Porras, A
Spiesman, W
Allen, LE
Blake, GA
Evans, NJ
Harvey, PM
Koerner, DW
Mundy, LG
Myers, PC
Padgett, DL
Sargent, AI
Stapelfeldt, KR
van Dishoeck, EF
Bertoldi, F
Chapman, N
Cieza, L
DeVries, CH
Ridge, NA
Wahhaj, Z
机构
[1] Univ Texas, Austin, TX 78712 USA
[2] Leiden Observ, NL-2300 RA Leiden, Netherlands
[3] Natl Radio Astron Observ, Socorro, NM 87801 USA
[4] Max Planck Inst Radioastron, D-5300 Bonn, Germany
[5] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[6] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[7] Korea Astron Observ, Taejon 305348, South Korea
[8] Harvard Smithsonian Ctr Astrophys, Submillimeter Array Project, Hilo, HI 96720 USA
[9] Max Planck Inst Astrophys, D-85741 Garching, Germany
[10] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA
[11] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[12] No Arizona Univ, Dept Phys & Astron, Flagstaff, AZ 86011 USA
[13] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA
[14] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
infrared : stars; ISM : individual (L1014); stars : formation; stars; low-mass; brown dwarfs;
D O I
10.1086/422818
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present observations of L1014, a dense core in the Cygnus region previously thought to be starless, but data from the Spitzer Space Telescope show the presence of an embedded source. We propose a model for this source that includes a cold core, heated by the interstellar radiation field, and a low-luminosity internal source. The low luminosity of the internal source suggests a substellar object. If L1014 is representative, other "starless'' cores may turn out to harbor central sources.
引用
收藏
页码:396 / 401
页数:6
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