A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey

From National Research Council Canada

DOI	Resolve DOI: https://doi.org/10.1093/mnras/stw301
Author	Search for: Marsh, K. A.; Search for: Kirk, J. M.; Search for: André, Ph.; Search for: Griffin, M. J.; Search for: Könyves, V.; Search for: Palmeirim, P.; Search for: Men'shchikov, A.; Search for: Ward-Thompson, D.; Search for: Benedettini, M.; Search for: Bresnahan, D. W.; Search for: Di Francesco, J.¹; Search for: Elia, D.; Search for: Motte, F.; Search for: Peretto, N.; Search for: Pezzuto, S.; Search for: Roy, A.; Search for: Sadavoy, S.; Search for: Schneider, N.; Search for: Spinoglio, L.; Search for: White, G. J.
Name affiliation	National Research Council Canada. National Science Infrastructure
Format	Text
Type	Article
Journal title	Monthly Notices of the Royal Astronomical Society
ISSN	0035-8711 1365-2966
Volume	459
Issue	1
Pages	342–356
Subject	Stars formation; Luminosity function; Mass function; ISM clouds; ISM individual objects; L1495; local interstellar matter; submillimetre
Abstract	We present a catalogue of dense cores in a ∼4° × 2° field of the Taurus star-forming region, inclusive of the L1495 cloud, derived from Herschel SPIRE and PACS observations in the 70 μm, 160 μm, 250 μm, 350 μm, and 500 μm continuum bands. Estimates of mean dust temperature and total mass are derived using modified blackbody fits to the spectral energy distributions. We detect 525 starless cores of which ∼10–20 per cent are gravitationally bound and therefore presumably prestellar. Our census of unbound objects is ∼85 per cent complete for M > 0.015 M⊙ in low-density regions (AV ≲ 5 mag), while the bound (prestellar) subset is ∼85 per cent complete for M > 0.1 M⊙ overall. The prestellar core mass function (CMF) is consistent with lognormal form, resembling the stellar system initial mass function, as has been reported previously. All of the inferred prestellar cores lie on filamentary structures whose column densities exceed the expected threshold for filamentary collapse, in agreement with previous reports. Unlike the prestellar CMF, the unbound starless CMF is not lognormal, but instead is consistent with a power-law form below 0.3 M⊙ and shows no evidence for a low-mass turnover. It resembles previously reported mass distributions for CO clumps at low masses (M ≲ 0.3 M⊙). The volume density PDF, however, is accurately lognormal except at high densities. It is consistent with the effects of self-gravity on magnetized supersonic turbulence. The only significant deviation from lognormality is a high-density tail which can be attributed unambiguously to prestellar cores.
Publication date	2016-02-10
Publisher	Oxford University Press
Language	English
Peer reviewed	Yes
NPARC number	23000380
Export citation	Export as RIS
Report a correction	Report a correction
Record identifier	70b2dde6-d187-4e33-950b-9b1346a40ce6
Record created	2016-07-12
Record modified	2020-03-16

Report a problem on this page

Date modified:: 2020-03-28