Multiwavelength observations of EXO 0748-676. II. Emission-line behavior

We present optical and ultraviolet spectra, light curves, and Doppler tomograms of the low-mass X-ray binary EXO 0748-676. Using an extensive set of 15 emission-line tomograms, we show that, along with the usual emission from the stream and "hot spot," there is extended nonaxisymmetric emi...

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Main Authors: Pearson, K, Hynes, R, Steeghs, D, Jonker, P, Haswell, C, King, A, O'Brien, K, Nelemans, G, Méndez, M
Format: Journal article
Language:English
Published: Institute of Physics Publishing 2006
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author Pearson, K
Hynes, R
Steeghs, D
Jonker, P
Haswell, C
King, A
O'Brien, K
Nelemans, G
Méndez, M
author_facet Pearson, K
Hynes, R
Steeghs, D
Jonker, P
Haswell, C
King, A
O'Brien, K
Nelemans, G
Méndez, M
author_sort Pearson, K
collection OXFORD
description We present optical and ultraviolet spectra, light curves, and Doppler tomograms of the low-mass X-ray binary EXO 0748-676. Using an extensive set of 15 emission-line tomograms, we show that, along with the usual emission from the stream and "hot spot," there is extended nonaxisymmetric emission from the disk rim. Some of the emission and Ha and Hβ absorption features lend weight to the hypothesis that part of the stream overflows the disk rim and forms a two phase medium. The data are consistent with a 1.35 M ⊙ neutron star with a main-sequence companion and hence a mass ratio q ≈ 0.34. © 2006. The American Astronomical Society. All rights reserved.
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spelling oxford-uuid:203fae14-7c7a-436f-9b65-75e701b2fe5e2022-03-26T11:26:25ZMultiwavelength observations of EXO 0748-676. II. Emission-line behaviorJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:203fae14-7c7a-436f-9b65-75e701b2fe5eEnglishSymplectic Elements at OxfordInstitute of Physics Publishing2006Pearson, KHynes, RSteeghs, DJonker, PHaswell, CKing, AO'Brien, KNelemans, GMéndez, MWe present optical and ultraviolet spectra, light curves, and Doppler tomograms of the low-mass X-ray binary EXO 0748-676. Using an extensive set of 15 emission-line tomograms, we show that, along with the usual emission from the stream and "hot spot," there is extended nonaxisymmetric emission from the disk rim. Some of the emission and Ha and Hβ absorption features lend weight to the hypothesis that part of the stream overflows the disk rim and forms a two phase medium. The data are consistent with a 1.35 M ⊙ neutron star with a main-sequence companion and hence a mass ratio q ≈ 0.34. © 2006. The American Astronomical Society. All rights reserved.
spellingShingle Pearson, K
Hynes, R
Steeghs, D
Jonker, P
Haswell, C
King, A
O'Brien, K
Nelemans, G
Méndez, M
Multiwavelength observations of EXO 0748-676. II. Emission-line behavior
title Multiwavelength observations of EXO 0748-676. II. Emission-line behavior
title_full Multiwavelength observations of EXO 0748-676. II. Emission-line behavior
title_fullStr Multiwavelength observations of EXO 0748-676. II. Emission-line behavior
title_full_unstemmed Multiwavelength observations of EXO 0748-676. II. Emission-line behavior
title_short Multiwavelength observations of EXO 0748-676. II. Emission-line behavior
title_sort multiwavelength observations of exo 0748 676 ii emission line behavior
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