Froebrich, C. (2005) Which Are the Youngest Protostars? Determining Properties of Confirmed and Candidate Class 0 Sources by Broadband Photometry. The Astrophysical Journal (Supplement Series), 156 (2). pp. 169-177. ISSN 0067-0049.
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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.
|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:||14 Jan 2010 14:01|
|Resource URI:||http://kar.kent.ac.uk/id/eprint/1154 (The current URI for this page, for reference purposes)|
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