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. (doi:10.1086/426441) (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:1154)

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://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
DOI/Identification number:	10.1086/426441
Subjects:	Q Science > QB Astronomy > QB460 Astrophysics
Divisions:	Divisions > Division of Natural Sciences > Physics and Astronomy
Depositing User:	Sara Witchell
Date Deposited:	19 Dec 2007 18:46 UTC
Last Modified:	05 Nov 2024 09:31 UTC
Resource URI:	https://kar.kent.ac.uk/id/eprint/1154 (The current URI for this page, for reference purposes)

University of Kent Author Information

Froebrich, Dirk.

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