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J/A+A/473/523 Determination of the mass of neutron stars (Van der Meer+, 2007)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
list.dat smcx1/* lmcx4/* cenx3/*
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/473/523
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drwxr-xr-x 14 cats archive 246 Jan 29 2012 [Up]
drwxr-xr-x 5 cats archive 323 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 493 Dec 19 2022 .message
-r--r--r-- 1 cats archive 4450 Dec 16 2007 ReadMe
drwxr-xr-x 2 cats archive 4096 Aug 4 2007 cenx3
-r--r--r-- 1 cats archive 3060 Oct 9 2007 list.dat [txt] [txt.gz] [fits] [fits.gz] [html]
drwxr-xr-x 2 cats archive 4096 Aug 4 2007 lmcx4
drwxr-xr-x 2 cats archive 4096 Aug 4 2007 smcx1 Beginning of ReadMe :J/A+A/473/523 Spectroscopic monitoring of 3 neutron stars (Van der Meer+, 2007)
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Determination of the mass of the neutron star in SMC X-1, LMC X-4 and Cen X-3
with VLT/UVES.
van der Meer A., Kaper L., van Kerkwijk M.H., Heemskerk M.H.M.,
van den Heuvel E.P.J.
<Astron. Astrophys. 473, 523 (2007)>
=2007A&A...473..523V
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ADC_Keywords: Binaries, eclipsing ; Pulsars ; Radial velocities
Keywords: stars: binaries: eclipsing - stars: neutron - stars: general -
equation of state - accretion, accretion disks
Abstract:
We present the results of a spectroscopic monitoring campaign of the
OB-star companions to the eclipsing X-ray pulsars SMC X-1, LMC X-4
and Cen X-3. High-resolution optical spectra obtained with UVES on
the ESO Very Large Telescope are used to determine the radial-velocity
orbit of the OB (super)giants with high precision. The excellent
quality of the spectra provides the opportunity to measure the
radial-velocity curve based on individual lines, and to study the
effect of possible distortions of the line profiles due to e.g. X-ray
heating on the derived radial-velocity amplitude.
Description:
Electronic tables belong to table 3 of the paper. As described in the
paper, all lines that have been fit to obtain the radial-velocity
curve of SMC X-1, LMC X-4 and Cen X-3, are published as online
material at CDS. Each table contains the orbital phase, the velocity,
error on the velocity, the full width at half maximum, error on the
full width at half maximum, the flux and error on the flux. Errors
indicate 1 sigma.
Objects:
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RA (2000) DE Designation(s) (Directory)
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01 17 05.1 -73 26 36 SMC X-1 = X SMC X-1 (smcx1)
05 32 49.9 -66 22 14 LMC X-4 = X LMC X-4 (lmcx4)
11 21 15.8 -60 37 23 Cen X-3 = V* V779 Cen (cenx3)
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