output
19962026
most citedAn accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907

464 citations

Showing astro-phShow all

9 papers · 1 filter

astro-ph2008★ 224 cited

A cosmic abundance standard: chemical homogeneity of the solar neighbourhood and the ISM dust-phase composition

Norbert Przybilla, Maria-Fernanda Nieva, Keith Butler

A representative sample of unevolved early B-type stars in nearby OB associations and the field is analysed to unprecedented precision using NLTE techniques. The resulting chemical…

astro-ph2007★ 93 cited

Pulse phase resolved analysis of the HMXB Cen X-3 over two binary orbits

S. Suchy, K. Pottschmidt, J. Wilms +7

We present a detailed analysis of observations of the high mass X-ray binary Cen X-3 spanning two consecutive binary orbits performed with the RXTE satellite in early March 1997. T…

astro-ph2005★ 1 cited

Exciting new features in the frequency spectrum of the EC14026 star HS0702+6043 - Simultaneous g-modes and p-modes in a sdB pulsator

S. Schuh, J. Huber, S. Dreizler +7

The discovery of a long-period g-mode oscillation in the previously known short-period p-mode sdB pulsator HS0702+6043 makes this star an extraordinary object, unique as a member o…

astro-ph2003★ 16 cited

The near-synchronous polar V1432 Aql (RX J1940.1-1025): Accretion geometry and synchronization time scale

R. Staubert, S. Friedrich, K. Pottschmidt +5

The magnetic Cataclysmic Variable (mCV) V1432 Aql (RX 1940.1-1025) belongs to the four-member subclass of near-synchronous polars with a slight non-synchronism (<2 %) between the s…

astro-ph2002★ 21 cited

A new two-pole accretion polar: RX J1846.9+5538

R. Schwarz, J. Greiner, G. H. Tovmassian +2

We report the discovery of a new, bright (V = 17 mag) AM Her system as the optical counterpart of the soft ROSAT All-Sky-Survey source RX J1846.9+5538 (= 1RXS J184659.4+553834). Op…

astro-ph2000

Saving Astronomical Treasures

Noah Brosch, Rene Hudec, Peter Kroll +1

The time domain is under-exploited in an astrophysical context, because the large photographic plate collections are almost never consulted by young astronomers. This is a result o…