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.
| The full text of this publication is not available from this repository. (Contact us about this Publication) |
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: | 14 Jan 2010 14:01 |
| Resource URI: | http://kar.kent.ac.uk/id/eprint/1154 (The current URI for this page, for reference purposes) |
- Depositors only (login required):
