The Spitzer c2d survey of nearby dense cores.: II.: Discovery of a low-luminosity object in the "evolved starless core" L1521F

被引:133
作者
Bourke, Tyler L.
Myers, Philip C.
Evans, Neal J., II
Dunham, Michael M.
Kauffmann, Jens
Shirley, Yancy L.
Crapsi, Antonio
Young, Chadwick H.
Huard, Tracy L.
Brooke, Timothy Y.
Chapman, Nicholas
Cieza, Lucas
Lee, Chang Won
Teuben, Peter
Wahhaj, Zahed
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[2] Univ Texas, Austin, TX 78712 USA
[3] Max Planck Inst Radioastron, D-53121 Bonn, Germany
[4] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[5] Leiden Observ, NL-2300 RA Leiden, Netherlands
[6] Nicholls State Univ, Thibodaux, LA 70310 USA
[7] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA
[8] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[9] Korea Astron & Space Sci Inst, Taejon 305348, South Korea
[10] No Arizona Univ, Dept Phys & Astron, Flagstaff, AZ 86011 USA
基金
美国国家航空航天局;
关键词
D O I
10.1086/508161
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present Spitzer Space Telescope observations of the "evolved starless core" L1521F that reveal the presence of a very low luminosity object (L < 0.07 L-circle dot). The object, L1521F-IRS, is directly detected at mid- infrared wavelengths (> 5 mu m), but only in scattered light at shorter infrared wavelengths, showing a bipolar nebula oriented east- west that is probably tracing an outflow cavity. The nebula strongly suggests that L1521F-IRS is embedded in the L1521F core. Thus, L1521F-IRS is similar to the recently discovered L1014-IRS and the previously known IRAM 04191 in its substellar luminosity and dense core environment. However, these objects differ significantly in their core density, core chemistry, and outflow properties, and some may be destined to be brown dwarfs rather than stars.
引用
收藏
页码:L37 / L40
页数:4
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