Clark, J. S.; Steele, I. A.; Coe, M. J. and Roche, P.
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|DOI (Digital Object Identifier) Link:||http://doi.org/10.1046/j.1365-8711.1998.01436.x|
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We present infrared spectroscopy of the Be /X-ray binary HDE 245770/A0535+26 obtained over the period 1992–1995. The spectra show significant variability, reflecting changes in the circumstellar environment during this time. A reduction in the flux observed in the Paschen series lines between 1993 December and 1994 September correlates with a similar reduction in both the strength of Ha and the optical continuum emission, which can be attributed to a reduction in the emission measure of the disc. A turnover between optically thin and thick emission is seen for both Paschen and Brackett series lines, and allows an estimate of the disc density as 11012 cmÃ�3. Echelle spectroscopy reveals strong similarities between the He I 1.008, 2.058 lm, Ha and Paschen series line profiles, suggesting their formation in a similar (and asymmetric) region of the disc. In contrast, the line profile of He I 6678 Â°A indicates that it is formed at smaller radii than the other transitions.
|Item Type:||Journal Article|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 9108 not found.|
|Date Deposited:||06 Jul 2009 12:42|
|Last Modified:||02 Aug 2016 16:12|
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