Search Publications

Magnetic helicity accumulation and tilt angle evolution of newly emerging active regions
DOI: 10.1051/0004-6361/200810032 Bibcode: 2009A&A...502..333Y

Zhang, H.; Yang, S.; Büchner, J.

Context: It has been known for years that there is a general dominance of negative (positive) helicity of active regions (ARs) in the northern (southern) solar hemisphere. For a better understanding of the role of helicity in the evolution of active regions, it is necessary to know more about the accumulation of helicity during the emergence of ac…

2009 Astronomy and Astrophysics
SOHO 33
A forming disk at z ~ 0.6: collapse of a gaseous disk or major merger remnant?
DOI: 10.1051/0004-6361:200810521 Bibcode: 2009A&A...493..899P

Yang, Y.; Neichel, B.; Flores, H. +2 more

Context: Local spiral galaxies contain roughly two-thirds of the present-day stellar mass density. However, the formation process of disks is still poorly understood.
Aims: We present and analyze observations of J033241.88-274853.9 at z = 0.6679 to understand how its stellar disk was formed.
Methods: We combine multi-wavelength EIS, HST/AC…

2009 Astronomy and Astrophysics
eHST 33
The architecture of the GJ 876 planetary system. Masses and orbital coplanarity for planets b and c
DOI: 10.1051/0004-6361/200811280 Bibcode: 2009A&A...496..249B

Bean, J. L.; Seifahrt, A.

We present a combined analysis of previously published high-precision radial velocities and astrometry for the GJ 876 planetary system using a self-consistent model that accounts for the planet-planet interactions. Assuming the three planets so far identified in the system are coplanar, we find that including the astrometry in the analysis does no…

2009 Astronomy and Astrophysics
eHST 33
XMM-Newton observation of the persistent Be/NS X-ray binary pulsar RX J1037.5-5647 in a low luminosity state
DOI: 10.1051/0004-6361/200912538 Bibcode: 2009A&A...505..947L

Tiengo, A.; Mereghetti, S.; Sidoli, L. +2 more

The spectra of several X-ray binary pulsars display a clear soft excess, which in most cases can be described with a blackbody model, above the main power-law component. While in the high-luminosity sources it is usually characterized by low temperature (kT < 0.5 keV) and a large emission radius (R > 100 km), in the two persistent and low-lu…

2009 Astronomy and Astrophysics
XMM-Newton 32
High-precision multi-band measurements of the angular clustering of X-ray sources
DOI: 10.1051/0004-6361/200911670 Bibcode: 2009A&A...500..749E

Ebrero, J.; Carrera, F. J.; Watson, M. G. +2 more

Aims: We aim to study the large-scale structure of an extragalactic serendipitous X-ray survey with unprecedented accuracy thanks to the large statistics involved, and provide insight into the environment of AGN at the epochs when their space density declines (z ∼ 1{-}2).
Methods: In this paper we present the two-point angular correlation func…

2009 Astronomy and Astrophysics
XMM-Newton 32
Phase-resolved XMM-Newton observations of the massive WR+O binary WR 22
DOI: 10.1051/0004-6361/20077981 Bibcode: 2009A&A...508..805G

Gosset, E.; Nazé, Y.; Rauw, G. +2 more

Aims. To better understand the phenomenon of colliding winds in massive binary stars, we study the X-ray lightcurve of a WR+O system of the Carina region, a system well known for the high mass of its primary.
Methods: Phase-resolved X-ray observations of the massive WR+O binary system WR 22 were performed with the XMM-Newton facility. We obser…

2009 Astronomy and Astrophysics
XMM-Newton 32
Probing variability patterns of the Fe K line complex in bright nearby AGNs
DOI: 10.1051/0004-6361/200912188 Bibcode: 2009A&A...507..159D

Cappi, M.; Ponti, G.; Iwasawa, K. +5 more

Context: The unprecedented sensitivity of current X-ray telescopes allows the issue of the Fe K line complex variability patterns in bright, nearby AGNs to be addressed for the first time. These kinds of studies have the potential to map the accretion flow in the strong gravity regime of supermassive black holes.
Aims: We examine XMM-Newton ob…

2009 Astronomy and Astrophysics
XMM-Newton 32
Pulsations in the late-type Be star HD 50 209 detected by CoRoT
DOI: 10.1051/0004-6361/200911901 Bibcode: 2009A&A...506..125D

Auvergne, M.; Poretti, E.; Michel, E. +22 more

Context: The presence of pulsations in late-type Be stars is still a matter of controversy. It constitutes an important issue to establish the relationship between non-radial pulsations and the mass-loss mechanism in Be stars.
Aims: To contribute to this discussion, we analyse the photometric time series of the B8IVe star HD 50 209 observed by…

2009 Astronomy and Astrophysics
CoRoT 32
Broad-band properties of the hard X-ray cataclysmic variables IGR J00234+6141 and 1RXS J213344.1+510725
DOI: 10.1051/0004-6361/200911816 Bibcode: 2009A&A...501.1047A

Mukai, K.; de Martino, D.; Terada, Y. +5 more

Context: A significant number of cataclysmic variables have been detected as hard X-ray sources in the INTEGRAL survey, most of them of the magnetic intermediate polar type.
Aims: We present a detailed X-ray broad-band study of two new sources, IGR J00234+6141 and 1RXS J213344.1+510725, that allow us to classify them as secure members of the i…

2009 Astronomy and Astrophysics
INTEGRAL Suzaku XMM-Newton 32
Solar transition region above sunspots
DOI: 10.1051/0004-6361/200912114 Bibcode: 2009A&A...505..307T

Marsch, E.; Curdt, W.; Teriaca, L. +2 more

Aims: We study the transition region (TR) properties above sunspots and the surrounding plage regions, by analyzing several sunspot reference spectra obtained by the SUMER (Solar Ultraviolet Measurements of Emitted Radiation) instrument in March 1999 and November 2006.
Methods: We compare the SUMER spectra observed in the umbra, penumbra, plag…

2009 Astronomy and Astrophysics
SOHO 32