output
19922026
Showing 2008 · astro-phShow all

198 papers · 2 filters

astro-ph2008★ 1 cited

Search for the magnetic field of the O7.5 III star xi Persei

H. F. Henrichs, R. S. Schnerr, J. A. de Jong +3

Cyclical wind variability is an ubiquitous but as yet unexplained feature among OB stars. The O7.5 III(n)((f)) star xi Persei is the brightest representative of this class on the N…

astro-ph2008★ 2 cited

The magnetic field of the B3V star 16 Pegasi

H. F. Henrichs, C. Neiner, R. S. Schnerr +8

The Slowly Pulsating B3V star 16 Pegasi was discovered by Hubrig (2006) to be magnetic, based on low-resolution spectropolarimetric observations with FORS1 at the VLT. We have conf…

astro-ph2008★ 15 cited

Discovery of non-radial pulsations in the spectroscopic binary Herbig Ae star RS Cha

T. Böhm, W. Zima, C. Catala +3

In this article we present a first discovery of non radial pulsations in both components of the Herbig Ae spectroscopic binary star RS Cha. The binary was monitored in quasi-contin…

astro-ph2008

The MiMeS Project: First Results

J. H. Grunhut, E. Alecian, D. A. Bohlender +11

Massive stars are those stars with initial masses above about 8 times that of the sun, eventually leading to catastrophic explosions in the form of supernovae. These represent the…

astro-ph2008

Discovery of fossil magnetic fields in the intermediate-mass pre-main sequence stars

E. Alecian, G. A. Wade, C. Catala

It is now well-known that the surface magnetic fields observed in cool, lower-mass stars on the main sequence (MS) are generated by dynamos operating in their convective envelopes.…

astro-ph2008★ 15 cited

Delayed Recombination and Standard Rulers

Francesco De Bernardis, Rachel Bean, Silvia Galli +3

Measurements of Baryonic Acoustic Oscillations in galaxy surveys have been recognized as a powerful tool for constraining dark energy. However, this method relies on the knowledge…