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  5. Herschel observations of B1-bS and B1-bN: two first hydrostatic core candidates in the Perseus star-forming cloud
 

Herschel observations of B1-bS and B1-bN: two first hydrostatic core candidates in the Perseus star-forming cloud

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2012
Author(s)
PEZZUTO, Stefano  
•
ELIA, Davide Quintino  
•
SCHISANO, EUGENIO  
•
Strafella, F.
•
Di Francesco, J.
•
Sadavoy, S.
•
André, P.
•
BENEDETTINI, Milena  
•
Bernard, J. P.
•
DI GIORGIO, Anna Maria  
•
Facchini, A.
•
Hennemann, M.
•
Hill, T.
•
Könyves, V.
•
MOLINARI, Sergio  
•
Motte, F.
•
Nguyen-Luong, Q.
•
Peretto, N.
•
Pestalozzi, M.
•
Polychroni, D.
•
RYGL, Kazi Lucie Jessica  
•
Saraceno, P.
•
Schneider, N.
•
SPINOGLIO, Luigi Giuseppe Maria  
•
TESTI, Leonardo  
•
Ward-Thompson, D.
•
White, G. J.
DOI
10.1051/0004-6361/201219501
Abstract
We report far-infrared Herschel observations obtained between 70 μm and 500 μm of two star-forming dusty condensations, [HKM99] B1-bS and [HKM99] B1-bN, in the B1 region of the Perseus star-forming cloud. In the western part of the Perseus cloud, B1-bS is the only source detected in all six PACS and SPIRE photometric bands, but it is not visible in the Spitzer map at 24 μm. B1-bN is clearly detected between 100 μm and 250 μm. We have fitted the spectral energy distributions of these sources to derive their physical properties, and find that a simple greybody model fails to reproduce the observed spectral energy distributions. At least a two-component model is required, consisting of a central source surrounded by a dusty envelope. The properties derived from the fit, however, suggest that the central source is not a Class 0 object. We then conclude that while B1-bS and B1-bN appear to be more evolved than a pre-stellar core, the best-fit models suggest that their central objects are younger than a Class 0 source. Hence, they may be good candidates to be examples of the first hydrostatic core phase. The projected distance between B1-bS and B1-bN is a few Jeans lengths. If their physical separation is close to this value, this pair would allow studying the mutual interactions between two forming stars at a very early stage of their evolution.

Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.Appendices are available in electronic form at http://www.aanda.org

Volume
547
Start page
A54
Uri
http://hdl.handle.net/20.500.12386/32978
Url
https://www.aanda.org/articles/aa/full_html/2012/11/aa19501-12/aa19501-12.html
http://arxiv.org/abs/1209.5290v1
Issn Identifier
0004-6361
Ads BibCode
2012A&A...547A..54P
Rights
open.access
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