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Symposium - International Astronomical Union
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Symposium - International Astronomical Union
Article . 1994 . Peer-reviewed
License: Cambridge Core User Agreement
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https://doi.org/10.1007/978-94...
Part of book or chapter of book . 1994 . Peer-reviewed
Data sources: Crossref
http://oro.open.ac.uk/40864/...
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Infrared spectroscopy of Be/X-ray binaries

descriptionPublicationkeyboard_double_arrow_right Article , Part of book or chapter of book , Other literature type 01 Jan 1994 English Publisher:Cambridge University Press (CUP)Journal:Symposium - International Astronomical Union, volume 162, pages 204-205 (issn: 0074-1809, Copyright policy )
Authors: Andrew Norton; S. J. Unger; P. Roche; M. J. Coe; C. Everall;

doi: 10.1017/s007418090021485x , 10.1007/978-94-011-1030-3_52

Infrared spectroscopy of Be/X-ray binaries

Abstract

We present infrared spectra of 4 Be/X-ray binaries in the K band, and 4 spectra in the J, H and K bands of 2 more sources. The HI IR emission lines are useful determinators of the conditions in the inner regions of the circumstellar disk about the Be star, due to optical depth effects. These are preliminary results, and hope to be followed up by high resolution echelle spectra, where we wish to estimate the velocity field, temperature and density structure of the circumstellar material.

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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