E. Fiorellino, D. Elia, Ph. Andrť, A. Men’shchikov, S. Pezzuto, E. Schisano, V. KŲnyves, D. Arzoumanian, M. Benedettini, D. Ward-Thompson, A. Bracco, J. Di Francesco, S. Bontemps, J. Kirk, F. Motte, S. Molinari
The Herschel Gould Belt survey mapped the nearby (d < 500 pc) star-forming regions to understand better how the prestellar phase influences the star formation process. Here, we report a complete census of dense cores in a ∼15 deg2 area of the Serpens star-forming region located between d ∼ 420 and 484 pc. The PACS and SPIRE cameras imaged this cloud from 70 to 500 μm. With the multiwavelength source extraction algorithm getsources, we extract 833 sources, of which 709 are starless cores and 124 are candidate protostellar cores. We obtain temperatures and masses for all the sample, classifying the starless cores in 604 prestellar cores and 105 unbound cores. Our census of sources is 80 per cent complete for M > 0.8 M⊙ overall. We produce the core mass function (CMF) and compare it with the initial mass function (IMF). The prestellar CMF is consistent with lognormal trend up to ∼2 M⊙, after which it follows a power law with slope of −2.05 ± 0.34. The tail of its CMF is steeper but still compatible with the IMF for the region we studied in this work. We also extract the filaments network of the Serpens region, finding that 81 per cent of prestellar cores lie on filamentary structures. The spatial association between cores and filamentary structure supports the paradigm, suggested by other Herschel observations, that prestellar cores mostly form on filaments. Serpens is confirmed to be a young, low-mass and active star-forming region.
stars: formation; ISM: clouds; ISM: individual (Serpens); ISM: structure; infrared: ISM; submillimetre: ISM; Astrophysics - Astrophysics of Galaxies; Astrophysics - Solar and Stellar Astrophysics
Monthly Notices of the Royal Astronomical Society
Volume 500, Issue 4, Page 4257