pith. sign in

arxiv: 0808.0898 · v1 · pith:QY3PH523new · submitted 2008-08-06 · 🌌 astro-ph

Ultraluminous X-ray Sources and Their Nebulae

classification 🌌 astro-ph
keywords nebulaesourcesenergyshock-poweredultraluminousx-rayappearbubble
0
0 comments X
read the original abstract

One of the interesting features of Ultraluminous X-ray sources is that many of them are surrounded by luminous nebulae exhibiting diverse observational properties. In different cases the nebulae are photoionized or shock-powered. Generally, the two energy sources appear to coexist. ULX bubble nebulae may be considered a new class of shock-powered nebulae similar to upscaled versions of stellar wind bubbles. Their expansion rates support constant energy influx rather than single powerful events like Hypernova explosions.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.