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 > Q Science (General) Q Science > QB Astronomy Q Science > QC Physics |
| Divisions: | Divisions > Division of Natural Sciences > Physics and Astronomy |
| Depositing User: | Sara Witchell |
| Date Deposited: | 19 Dec 2007 18:46 UTC |
| Last Modified: | 16 Nov 2021 09:40 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/1154 (The current URI for this page, for reference purposes) |
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