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.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Similar content being viewed by others
References
André, P., Ward-Thompson, D., & Barsony, M. 1993, ApJ, 406, 122
Liseau, R. et al. 1999, A&A, 344, 342
Motte, F., André, P., & Neri, R. 1998, A&A, 336, 150
Stamatellos, D. & Whitworth, A. P. 2003, A&A, 407, 941
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2005 Springer
About this paper
Cite this paper
Stamatellos, D., Whitworth, A. (2005). How Well Determined is the Core Mass Function of ρ OPH?. In: Corbelli, E., Palla, F., Zinnecker, H. (eds) The Initial Mass Function 50 Years Later. Astrophysics and Space Science Library, vol 327. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-3407-7_60
Download citation
DOI: https://doi.org/10.1007/978-1-4020-3407-7_60
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-3406-0
Online ISBN: 978-1-4020-3407-7
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)