Talk:RCW 103
Appearance
This article is rated Stub-class on Wikipedia's content assessment scale. It is of interest to the following WikiProjects: | ||||||||||||||
|
Typoe in the coordinates.
[edit]SIMBAD, Uranometria and other proven reliable sources list the degree compoment of the Declination as -51 rather than -52 degrees.
I know nothing about astrophysics, but it seems that this article can be expanded
[edit]So here are a few citations (including the one currently listed in the external links) for any future editor who wants to take a crack at it.
- Gotthelf, E.V.; Petre, R.; Hwang, U. (October 1997). "The Nature of the Radio-quiet Compact X-Ray Source in Supernova Remnant RCW 103" (PDF). The Astrophysical Journal. 487 (2): L175–L179. arXiv:astro-ph/9707035. Bibcode:1997ApJ...487L.175G. doi:10.1086/310900.
- Carter, Lynn M.; Dickel, John R.; Bomans, Dominik J. (September 1997). "Expansion of the Supernova Remnant RCW 103". Publications of the Astronomical Society of the Pacific. 109 (793): 990–997. Bibcode:1997PASP..109..990C. doi:10.1086/133971. JSTOR 40680993.
- "RCW 103: A Star With a Mystery Partner?". NASA. 10 July 2007. Archived from the original on 25 June 2017.
- Dickel, John R.; Green, Anne; Ye, Taisheng; D.K., Milne (January 1996). "The Supernova Remnant RCW 103 at Radio Wavelengths". Astronomical Journal. 111: 340. Bibcode:1996AJ....111..340D. doi:10.1086/117786.
- Pizzolato, Fabio; Colpi, Monica; de Luca, Andrea; Mereghetti, Sandro; Tiengo, Andrea (February 2008). "1E161348-5055 in the Supernova Remnant RCW 103: A Magnetar in a Young Low Mass Binary System?". 40 Years of Pulsars : Millisecond Pulsars, Magnetars and More. AIP Conference Proceedings. Vol. 983. Springer. pp. 328–330. arXiv:0803.1373v1. Bibcode:2008AIPC..983..328P. doi:10.1063/1.2900176. ISBN 978-0735405028.