Aims. We intended to measure the radial velocity curve of the supergiant companion to the eclipsing high mass X-ray binary pulsar EXO 1722–36
High Mass X-ray Binaries consist of a neutron star or black-hole accreting material from its early-t...
We present Very Large Telescope (VLT) intermediate resolution spectroscopy of UY Vol, the optical co...
and other research outputs Preliminary determinations of the masses of the neu-tron star and mass do...
Aims. We intended to measure the radial velocity curve of the supergiant companion to the eclipsing ...
Aims. We intended to measure the radial velocity curve of the supergiant companion to the eclipsing ...
Aims. We report near-infrared observations of the supergiant donor to the eclipsing high mass X-ray ...
We report near-infrared radial velocity (RV) measurements of the recently identified donor star in t...
We present the results of a spectroscopic monitoring campaign of the OB-star companions to the ecli...
Abstract: The maximum mass of a neutron star (NS) is poorly defined. Theoretical attempts to define ...
We present optical spectroscopic measurements of the eclipsing high-mass X-ray binary (HMXB) XMMU J0...
We report near-infrared radial velocity (RV) measurements of the recently identified donor star in t...
International audienceAccurate measurements of the masses of neutron stars are necessary to test bin...
The most massive neutron stars constrain the behavior of ultra-dense matter, with larger masses poss...
The X-ray is a type of electromagnetic radiation which wavelength covers from 10nm to 0.01nm. They b...
Timing observations of the 38 s accreting X-ray pulsar OAO 1657-415 made with the BATSE large-area d...
High Mass X-ray Binaries consist of a neutron star or black-hole accreting material from its early-t...
We present Very Large Telescope (VLT) intermediate resolution spectroscopy of UY Vol, the optical co...
and other research outputs Preliminary determinations of the masses of the neu-tron star and mass do...
Aims. We intended to measure the radial velocity curve of the supergiant companion to the eclipsing ...
Aims. We intended to measure the radial velocity curve of the supergiant companion to the eclipsing ...
Aims. We report near-infrared observations of the supergiant donor to the eclipsing high mass X-ray ...
We report near-infrared radial velocity (RV) measurements of the recently identified donor star in t...
We present the results of a spectroscopic monitoring campaign of the OB-star companions to the ecli...
Abstract: The maximum mass of a neutron star (NS) is poorly defined. Theoretical attempts to define ...
We present optical spectroscopic measurements of the eclipsing high-mass X-ray binary (HMXB) XMMU J0...
We report near-infrared radial velocity (RV) measurements of the recently identified donor star in t...
International audienceAccurate measurements of the masses of neutron stars are necessary to test bin...
The most massive neutron stars constrain the behavior of ultra-dense matter, with larger masses poss...
The X-ray is a type of electromagnetic radiation which wavelength covers from 10nm to 0.01nm. They b...
Timing observations of the 38 s accreting X-ray pulsar OAO 1657-415 made with the BATSE large-area d...
High Mass X-ray Binaries consist of a neutron star or black-hole accreting material from its early-t...
We present Very Large Telescope (VLT) intermediate resolution spectroscopy of UY Vol, the optical co...
and other research outputs Preliminary determinations of the masses of the neu-tron star and mass do...
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