activity
19982026
most citedA natural explanation for periodic X-ray outbursts in Be/X-ray binaries

312 citations · 6.5k across the 153 of their papers we have counts for

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Showing 2004Show all

6 papers · 1 filter

astro-ph2004★ 3 cited

Massive X-ray binaries: New developments in the INTEGRAL era

Ignacio Negueruela

The study of massive X-ray binaries provides important observational diagnostics for a number of fundamental astrophysical issues, such as the evolution of massive stars, the stell…

astro-ph2004★ 1 cited

Be/X-ray binaries: An observational approach

Ignacio Negueruela

Be/X-ray binaries are the most numerous class of X-ray binaries. They constitute an excellent tracer of star formation and can be used to study several aspects of astrophysics, fro…

astro-ph2004★ 29 cited

A Period and a Prediction for the Of?p Spectrum Alternator HD 191612

Nolan R. Walborn, Ian D. Howarth, Gregor Rauw +7

The observational picture of the enigmatic O-type spectrum variable HD191612 has been sharpened substantially. A symmetrical, low-amplitude light curve with a period near 540 d has…

astro-ph2004★ 60 cited

On the class of Oe stars

Ignacio Negueruela, Iain A. Steele, Guillem Bernabeu

We present high-quality spectra of the majority of stars that have been classified as Oe and find that their published spectral types are generally too early, most likely due to in…

astro-ph2004★ 54 cited

Evidence for a Neutron Star in the non-pulsating massive X-ray binary 4U2206+54

J. M. Torrejón, I. Kreykenbohm, A. Orr +2

We present an analysis of archival RXTE and BeppoSAX data of the X-ray source 4U2206+54 . For the first time, high energy data (> 30 kev) are analyzed for this source. The data are…

astro-ph2004

A Search for Luminous Be stars

Ignacio Negueruela

As Be stars are restricted to luminosity classes III-V, but early B-type stars are believed to evolve into supergiants, it is to be expected that the Be phenomenon disappears at so…