Stamatelos, Dimitrios and Whitworth, Anthony Peter ![]() |
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 |
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Date Type: | Publication |
Status: | Published |
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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