Stamatelos, Dimitrios and Whitworth, Anthony Peter ORCID: https://orcid.org/0000-0002-1178-5486
2005.
How well determined is the core mass function of ρ Oph?
Corbelli, E., Palla, F. and Zinnecker, H., eds.
The initial mass function 50 years later,
Astrophysics and Space Science Library,
vol. 327.
Dordrecht:
Springer,
pp. 319-320.
(10.1007/978-1-4020-3407-7_60)
|
Official URL: http://link.springer.com/chapter/10.1007/978-1-402...
Abstract
Modeling of ρ Oph A indicates that the heating of the clump is mainly due to radiation from HD147889, a nearby star, which heats the clump to temperatures between 7 and 27 K. However, most of the clump volume is colder than 15 K.
| Item Type: | Book Section |
|---|---|
| Date Type: | Publication |
| Status: | Published |
| Schools: | Schools > Physics and Astronomy |
| Subjects: | Q Science > QB Astronomy |
| Publisher: | Springer |
| ISBN: | 9781402034060 |
| Last Modified: | 25 Oct 2022 09:39 |
| URI: | https://orca.cardiff.ac.uk/id/eprint/59489 |
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