Phase - resolved spectroscopy of the low - mass X - ray binaries 1636 - 536 / V 801 Arae and 1735 - 444 / V 926 Scorpii ?
نویسنده
چکیده
We present phase-resolved spectroscopy of the optical counterparts V 801 Ara and V 926 Sco of the low-mass X-ray binaries 1636-536 and 1735-444. To assist in the interpretation of the spectroscopic observations we derive new ephemerides for the photometric variations of both sources. Superior conjunction of the line emission region occurs at photometric phase ∼0.7 in both sources, which indicates that these variations are dominated by a component originating from the point where the mass stream from the donor star intersects the outer disk. We find that the properties of 1636-536/V 801 Ara and 1735-444/V 926 Sco are very similar.
منابع مشابه
Detection of the Irradiated Donor in the LMXBs 4 U 1636 - 536 ( = V 801
Phase-resolved VLT spectroscopy of the bursting Low Mass X-ray Binaries 4U 1636536/V801 Ara and 4U 1735-444/V926 Sco is presented. Doppler images of the NIII λ4640 Bowen transition reveal compact spots which we attribute to fluorescent emission from the donor star and enable us to define a new set of spectroscopic ephemerides. We measure Kem = 277 ± 22 km s and Kem = 226 ± 22 km s from the NIII...
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Phase-resolved VLT spectroscopy of the bursting Low Mass X-ray Binaries 4U 1636536/V801 Ara and 4U 1735-444/V926 Sco is presented. Doppler images of the NIII λ4640 Bowen transition reveal compact spots which we attribute to fluorescent emission from the donor star and enable us to define a new set of spectroscopic ephemerides. We measure Kem = 277 ± 22 km s and Kem = 226 ± 22 km s from the NIII...
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