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![]() I'm under the impression that all stars have stellar atmospheres, although in the case of dense objects like neutron stars the thickness of the atmosphere might be very small. What I would like to know is what the composition of the stellar atmosphere is in the case of various kinds of collapsed stars, such as neutron stars, kaon stars and black holes. Naturally, I don't expect anyone really to know in some of these cases where there is no experimental evidence, but in those cases I'd like to know what theory predicts for the composition of the stellar atmosphere. If you know of literature on this topic, please let me know. Ignorantly, Allan Adler ************************************************** ************************** * * * Disclaimer: I am a guest and *not* a member of the MIT Artificial * * Intelligence Lab. My actions and comments do not reflect * * in any way on MIT. Moreover, I am nowhere near the Boston * * metropolitan area. * * * ************************************************** ************************** |
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"AA" == Allan Adler writes:
AA I'm under the impression that all stars have stellar atmospheres, AA although in the case of dense objects like neutron stars the AA thickness of the atmosphere might be very small. What I would like AA to know is what the composition of the stellar atmosphere is in AA the case of various kinds of collapsed stars, such as neutron AA stars, kaon stars and black holes. Of course, black holes don't have a surface so they cannot have an "atmosphere" as one usually thinks of it. As for neutron stars, there is an extensive literature. For instance, typing in "neutron star atmosphere" at the ADS finds over 350 hits. Indeed, it looks like there are claims of direct detection of a neutron star atmosphere in 1E 1207.4-5209 via X-ray absorption features (Sanwal et al. 2002ApJ...574L..61S, URL: http://adsabs.harvard.edu/cgi-bin/np...pJ...574L..61S ). -- Lt. Lazio, HTML police | e-mail: No means no, stop rape. | http://patriot.net/%7Ejlazio/ sci.astro FAQ at http://sciastro.astronomy.net/sci.astro.html |
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