AX J0049.4-7323 - a close look at a neutron star interacting with a circumstellar disk
arXiv:astro-ph/0402031 · doi:10.1111/j.1365-2966.2004.07696.x
Abstract
Detailed evidence on the system AX J0049.4-7323 is presented here to show how the passage of the neutron star in the binary system disrupts the circumstellar disk of the mass donor Be star. A similar effect is noted in three other Be/X-ray binary systems. Together the observational data should provide valuable tools for modelling these complex interactions.
arXiv comment4 pages, accepted for publication in MNRAS
References in corpus (8)
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- INTEGRAL deep observations of the Small Magellanic Cloud
- Highly absorbed X-ray binaries in the Small Magellanic Cloud
- The newly discovered Be/X-ray binary Swift J004516.6-734703 in the SMC: witnessing the emergence of a circumstellar disc
- In-depth study of long-term variability in the X-ray emission of the Be/X-ray binary system AX J0049.4-7323
- Photometric Observations of Three High Mass X-Ray Binaries and a Search for Variations Induced by Orbital Motion
- The Be/neutron star system Swift J004929.5-733107 in the Small Magellanic Cloud -- X-ray characteristics and optical counterpart candidates
- X-ray and optical monitoring of the December 2017 outburst of the Be/X-ray binary AX J0049.4-7323