Herschel gould belt survey in Taurus - II. a census of dense cores and filaments in the TMC1 region

Kirk, J. M., Ward-Thompson, D., Di Francesco, J., André, Ph., Bresnahan, D. W., Könyves, V., Marsh, K. ORCID: https://orcid.org/0000-0003-0107-7803, Griffin, M. J. ORCID: https://orcid.org/0000-0002-0033-177X, Schneider, N., Men'shchikov, A., Palmeirim, P., Bontemps, S., Arzoumanian, D., Benedettini, M.. and Pezzuto, S 2024. Herschel gould belt survey in Taurus - II. a census of dense cores and filaments in the TMC1 region. Monthly Notices of the Royal Astronomical Society 532 (4) , pp. 4661-4680. 10.1093/mnras/stae1633

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Abstract

We present a catalogue of dense cores and filaments in a 3.8○ × 2.4○ field around the TMC1 region of the Taurus Molecular Cloud. The catalogue was created using photometric data from the Herschel SPIRE and PACS instruments in the 70 μm, 160 μm, 250 μm, 350 μm, and 500 μm continuum bands. Extended structure in the region was reconstructed from a Herschel column density map. Power spectra and PDFs of this structure are presented. The PDF splits into log-normal and power-law forms, with the high-density power-law component associated primarily with the central part of TMC1. The total mass in the mapped region is 2000 M⊙, of which 34% is above an extinction of AV ∼ 3 mag – a level that appears as a break in the PDF and as the minimum column density at which dense cores are found. A total of 35 dense filaments were extracted from the column density map. These have a characteristic FWHM width of 0.07 pc, but the TMC1 filament itself has a mean FWHM of ∼0.13 pc. The thermally supercritical filaments in the region are aligned orthogonal to the prevailing magnetic field direction. Derived properties for the supercritical TMC1 filament support the scenario of it being relatively young. A catalogue of 44 robust and candidate prestellar cores is created and is assessed to be complete down to 0.1 M⊙. The combined prestellar CMF for the TMC1 and L1495 regions is well fit by a single log-normal distribution and is comparable to the standard IMF.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Publisher:	Oxford University Press
ISSN:	0035-8711
Funders:	UKSA, STFC
Date of First Compliant Deposit:	8 July 2024
Date of Acceptance:	26 June 2024
Last Modified:	04 Sep 2024 13:15
URI:	https://orca.cardiff.ac.uk/id/eprint/170431

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