Search Publications

Accurate fundamental parameters for 23 bright solar-type stars
DOI: 10.1111/j.1365-2966.2010.16575.x Bibcode: 2010MNRAS.405.1907B

Butler, R. P.; Carrier, F.; Lo Curto, G. +7 more

We combine results from interferometry, asteroseismology and spectroscopy to determine accurate fundamental parameters of 23 bright solar-type stars, from spectral type F5 to K2 and luminosity classes III-V. For some stars we can use direct techniques to determine the mass, radius, luminosity and effective temperature, and we compare with indirect…

2010 Monthly Notices of the Royal Astronomical Society
IUE 251
Detection of a magnetic field on HD108: clues to extreme magnetic braking and the Of?p phenomenon
DOI: 10.1111/j.1365-2966.2010.17005.x Bibcode: 2010MNRAS.407.1423M

Bouret, J. -C.; Martins, F.; Donati, J. -F. +5 more

We report the detection of a magnetic field on the Of?p star HD108. Spectropolarimetric observations conducted in 2007, 2008 and 2009, respectively, with NARVAL@Télescope Bernard Lyot (TBL) and Echelle SpectroPolarimetric Device for the Observation of Stars at Canada-France-Hawaii Telescope (ESPaDOnS@CFHT) reveal a clear Zeeman signature in the av…

2010 Monthly Notices of the Royal Astronomical Society
IUE 90
Discovery of a strong magnetic field in the rapidly rotating B2Vn star HR 7355
DOI: 10.1111/j.1745-3933.2010.00857.x Bibcode: 2010MNRAS.405L..51O

Manset, N.; Wade, G. A.; Marcolino, W. L. F. +5 more

We report the detection of a strong, organized magnetic field in the He-variable early B-type star HR 7355 using spectropolarimetric data obtained with ESPaDOnS on the 3.6-m Canada-France-Hawaii Telescope within the context of the Magnetism in Massive Stars (MiMeS) Large Program. HR 7355 is both the most rapidly rotating known main-sequence magnet…

2010 Monthly Notices of the Royal Astronomical Society
Hipparcos IUE 53
Stellar winds and mass loss from extreme helium stars
DOI: 10.1111/j.1365-2966.2010.16410.x Bibcode: 2010MNRAS.404.1698J

Hamann, W. -R.; Jeffery, C. S.

Extreme helium stars are very rare low-mass supergiants in a late stage of evolution. They are probably contracting to become white dwarfs following a violent phase of evolution which caused them to become hydrogen-deficient giants, possibly R CrB stars. Using the latest generation of models for spherically expanding stellar atmospheres, we set ou…

2010 Monthly Notices of the Royal Astronomical Society
IUE eHST 40
A study of the interacting binary V393Scorpii
DOI: 10.1111/j.1365-2966.2010.16588.x Bibcode: 2010MNRAS.405.1947M

Mennickent, R. E.; Kołaczkowski, Z.; Graczyk, D. +1 more

We present high-resolution J-band spectroscopy of V393Sco obtained with the Cryogenic High-Resolution Infrared Echelle Spectrograph (CRIRES) at the ESO Paranal Observatory along with a discussion of archival International Ultraviolet Explorer (IUE) spectra and published broad-band magnitudes. The best fit to the spectral energy distribution outsid…

2010 Monthly Notices of the Royal Astronomical Society
IUE 15
Ultraviolet study of the active interacting binary star R Arae using archival IUE data
DOI: 10.1111/j.1365-2966.2009.15741.x Bibcode: 2010MNRAS.401..913R

Sahade, Jorge; Guinan, Edward F.; Reed, Phillip A. +7 more

The eclipsing and strongly interacting binary star system R Arae (HD 149730) is in a very active and very short-lived stage of its evolution. R Ara consists of a B9V primary and an unknown secondary. We have collected the International Ultraviolet Explorer (IUE) archival data on R Ara, with most of the data being studied for the first time. There …

2010 Monthly Notices of the Royal Astronomical Society
IUE 9
A far-ultraviolet variability survey of the globular cluster M80
DOI: 10.1111/j.1365-2966.2010.16729.x Bibcode: 2010MNRAS.406.1084T

Knigge, C.; Long, K. S.; Zurek, D. R. +2 more

We have searched for variable sources in the core region of M80, using far-ultraviolet (FUV) data taken with the Advanced Camera for Surveys on board the Hubble Space Telescope. We found three sources that exhibit strong signs of variability in our data. Among these is source TDK1, which we believe to be an RRLyrae star that reached maximum bright…

2010 Monthly Notices of the Royal Astronomical Society
IUE eHST 8
The dense and asymmetric central star wind of the young PN He 2-138
DOI: 10.1111/j.1365-2966.2009.15928.x Bibcode: 2010MNRAS.402..641P

Prinja, R. K.; Urbaneja, M. A.; Massa, D. L. +1 more

We present optical European Southern Observatory time series and UV archival (Far Ultraviolet Spectroscopic Explorer (FUSE), Hubble Space Telescope, International Ultraviolet Explorer) spectroscopy of the H-rich central star of He 2-138. Our study targets the central star wind in a very young planetary nebula, and explores physical conditions that…

2010 Monthly Notices of the Royal Astronomical Society
IUE eHST 3