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Low-energy absorption towards the ultra-compact binary 4U1850-087 located in the globular cluster NGC6712

L. Sidoli·N. La Palombara·T. Oosterbroek·A. N. Parmar
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Abstract

We report the results of two XMM-Newton observations of the ultra-compact low-mass X-ray binary 4U1850-087 located in the galactic globular cluster NGC6712. A broad emission feature at 0.7keV was detected in an earlier ASCA observation and explained as the result of an unusual Ne/O abundance ratio in the absorbing material local to the source. We find no evidence for this feature and derive Ne/O ratios in the range 0.14-0.21, consistent with that of the interstellar medium. During the second observation, when the source was 10% more luminous, there is some evidence for a slightly higher Ne/O ratio and additional absorption. Changes in the Ne/O abundance ratio have been detected from another ultra-compact binary, 4U1543-624. We propose that these changes result from an X-ray induced wind which is evaporated from an O and Ne rich degenerate donor. As the source X-ray intensity increases so does the amount of evaporation and hence the column densities and abundance ratio of Ne and O.

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L. Sidoli, N. La Palombara, T. Oosterbroek, A. N. Parmar. 2005-07-11. Low-energy absorption towards the ultra-compact binary 4U1850-087 located in the globular cluster NGC6712. https://doi.org/10.1051/0004-6361%3A20053438

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