Which Are the Youngest Protostars? Determining Properties of Confirmed and Candidate Class 0 Sources by Broadband Photometry

Froebrich, Dirk (2005) Which Are the Youngest Protostars? Determining Properties of Confirmed and Candidate Class 0 Sources by Broadband Photometry. Astrophysical Journal Supplement Series, 156 (2). pp. 169-177. ISSN 0067-0049. (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)

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. (Contact us about this Publication)
Official URL
http://dx.doi.org/10.1086/426441

Abstract

The most up to date and comprehensive catalogue of Class 0 protostars and their observational properties. Its data is made publicly available to the entire astronomical community via a widely used web page. It allowed us to discover some protostars have a significantly different time evolution of their mass accretion rate, caused by the environment they are forming in.

Item Type: Article
Subjects: Q Science > Q Science (General)
Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculties > Science Technology and Medical Studies > School of Physical Sciences
Depositing User: Sara Witchell
Date Deposited: 19 Dec 2007 18:46
Last Modified: 22 Apr 2014 13:30
Resource URI: https://kar.kent.ac.uk/id/eprint/1154 (The current URI for this page, for reference purposes)
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