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Triggered star formation within the bright-rimmed cloud SFO 75

Urquhart, J.S., Thompson, M.A., Morgan, L.K., White, Glenn J. (2006) Triggered star formation within the bright-rimmed cloud SFO 75. In: Proceedings of the International Astronomical Union. 2 (S237). (doi:10.1017/S1743921307002712) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:52249)

The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided.
Official URL:
http://www.dx.doi.org/10.1017/S1743921307002712

Abstract

We present the results of a multi-wavelength line and continuum study of the bright-rimmed cloud SFO 75 in an attempt to determine whether the ionisation front and its associated shocks, driven by the nearby O star, have triggered the formation of a new generation of stars within this bright-rimmed cloud. © 2007 International Astronomical Union.

Item Type: Conference or workshop item (Proceeding)
DOI/Identification number: 10.1017/S1743921307002712
Uncontrolled keywords: Radio continuum: stars, Stars: formation, Stars: pre-main sequence
Subjects: Q Science > QB Astronomy > QB460 Astrophysics
Divisions: Divisions > Division of Natural Sciences > Physics and Astronomy
Depositing User: James Urquhart
Date Deposited: 30 Nov 2015 16:57 UTC
Last Modified: 05 Nov 2024 10:38 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/52249 (The current URI for this page, for reference purposes)

University of Kent Author Information

Urquhart, J.S..

Creator's ORCID: https://orcid.org/0000-0002-1605-8050
CReDIT Contributor Roles:

Thompson, M.A..

Creator's ORCID:
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