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How well determined is the core mass function of ρ Oph?

Stamatelos, Dimitrios and Whitworth, Anthony Peter 2005. How well determined is the core mass function of ρ Oph? In: 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)

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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: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Publisher: Springer
ISBN: 9781402034060
Last Modified: 04 Jun 2017 06:23
URI: http://orca.cf.ac.uk/id/eprint/59489

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