Abstract
Infrared images of the dark cloud core B59 were obtained with the Spitzer Space Telescope as part of the "Cores to Disks" Legacy Science project. Photometry from 3.6-70 μm indicates at least 20 candidate low-mass young stars near the core, more than doubling the previously known population. Out of this group, 13 are located within ∼0.1 pc in projection of the molecular gas peak, where a new embedded source is detected. Spectral energy distributions span the range from small excesses above photospheric levels to rising in the mid-infrared. One other embedded object, probably associated with the millimeter source B59-MMS1, with a bolometric luminosity Lbol ∼ 2 L⊙, has extended structure at 3.6 and 4.5 μm, possibly tracing the edges of an outflow cavity. The measured extinction through the central part of the core is AV ≳, 45 mag. The B59 core is producing young stars with a high efficiency.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 364-374 |
| Number of pages | 11 |
| Journal | Astrophysical Journal |
| Volume | 655 |
| Issue number | 1 I |
| DOIs | |
| State | Published - Jan 20 2007 |
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Keywords
- Infrared: ISM
- Infrared: stars
- ISM: clouds
- Stars: pre-main-sequence
ASJC Scopus subject areas
- Space and Planetary Science
Cite this
The spitzer c2d survey of nearby dense cores. IV. Revealing the embedded cluster in B59. / Brooke, Timothy Y.; Huard, Tracy L.; Bourke, Tyler L.; Boogert, A. C Adwin; Allen, Lori E.; Blake, Geoffrey A.; Evans, Neal J.; Harvey, Paul M.; Koerner, David W; Mundy, Lee G.; Myers, Philip C.; Padgett, Deborah L.; Sargent, Anneila I.; Stapelfeldt, Karl R.; Van Dishoeck, Ewine F.; Chapman, Nicholas; Cieza, Lucas; Dunham, Michael M.; Lai, Shih Ping; Porras, Alicia; Spiesman, William; Teuben, Peter J.; Young, Chadwick H.; Wahhaj, Zahed; Lee, Chang Won.
In: Astrophysical Journal, Vol. 655, No. 1 I, 20.01.2007, p. 364-374.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - The spitzer c2d survey of nearby dense cores. IV. Revealing the embedded cluster in B59
AU - Brooke, Timothy Y.
AU - Huard, Tracy L.
AU - Bourke, Tyler L.
AU - Boogert, A. C Adwin
AU - Allen, Lori E.
AU - Blake, Geoffrey A.
AU - Evans, Neal J.
AU - Harvey, Paul M.
AU - Koerner, David W
AU - Mundy, Lee G.
AU - Myers, Philip C.
AU - Padgett, Deborah L.
AU - Sargent, Anneila I.
AU - Stapelfeldt, Karl R.
AU - Van Dishoeck, Ewine F.
AU - Chapman, Nicholas
AU - Cieza, Lucas
AU - Dunham, Michael M.
AU - Lai, Shih Ping
AU - Porras, Alicia
AU - Spiesman, William
AU - Teuben, Peter J.
AU - Young, Chadwick H.
AU - Wahhaj, Zahed
AU - Lee, Chang Won
PY - 2007/1/20
Y1 - 2007/1/20
N2 - Infrared images of the dark cloud core B59 were obtained with the Spitzer Space Telescope as part of the "Cores to Disks" Legacy Science project. Photometry from 3.6-70 μm indicates at least 20 candidate low-mass young stars near the core, more than doubling the previously known population. Out of this group, 13 are located within ∼0.1 pc in projection of the molecular gas peak, where a new embedded source is detected. Spectral energy distributions span the range from small excesses above photospheric levels to rising in the mid-infrared. One other embedded object, probably associated with the millimeter source B59-MMS1, with a bolometric luminosity Lbol ∼ 2 L⊙, has extended structure at 3.6 and 4.5 μm, possibly tracing the edges of an outflow cavity. The measured extinction through the central part of the core is AV ≳, 45 mag. The B59 core is producing young stars with a high efficiency.
AB - Infrared images of the dark cloud core B59 were obtained with the Spitzer Space Telescope as part of the "Cores to Disks" Legacy Science project. Photometry from 3.6-70 μm indicates at least 20 candidate low-mass young stars near the core, more than doubling the previously known population. Out of this group, 13 are located within ∼0.1 pc in projection of the molecular gas peak, where a new embedded source is detected. Spectral energy distributions span the range from small excesses above photospheric levels to rising in the mid-infrared. One other embedded object, probably associated with the millimeter source B59-MMS1, with a bolometric luminosity Lbol ∼ 2 L⊙, has extended structure at 3.6 and 4.5 μm, possibly tracing the edges of an outflow cavity. The measured extinction through the central part of the core is AV ≳, 45 mag. The B59 core is producing young stars with a high efficiency.
KW - Infrared: ISM
KW - Infrared: stars
KW - ISM: clouds
KW - Stars: pre-main-sequence
UR - http://www.scopus.com/inward/record.url?scp=33846859762&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=33846859762&partnerID=8YFLogxK
U2 - 10.1086/510115
DO - 10.1086/510115
M3 - Article
AN - SCOPUS:33846859762
VL - 655
SP - 364
EP - 374
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 1 I
ER -