Search Publications

INTEGRAL detection of a long powerful burst from SLX 1735-269
DOI: 10.1051/0004-6361:20041846 Bibcode: 2005A&A...434.1069M

Sunyaev, R.; Revnivtsev, M.; Lutovinov, A. +1 more

We present results of an analysis of the bursting behavior of the low mass X-ray binary system SLX 1735-269 during INTEGRAL observations of the Galactic Center region in 2003. Six type-I X-ray bursts were detected in total with one being much longer and more powerful then the others. A strong dependence of the burst recurrence time on the mass acc…

2005 Astronomy and Astrophysics
INTEGRAL 41
Interstellar Ca II Line Intensities and the Distances of the OB stars
DOI: 10.1086/496916 Bibcode: 2005ApJ...634..451M

Galazutdinov, G. A.; Han, Inwoo; Strobel, A. +4 more

We show that the equivalent widths of the well-known interstellar Ca II H and K lines can be used to determine the distances to OB stars in our Galaxy. The equivalent widths, measured in the spectra of 147 early-type stars, are strongly related to the Hipparcos parallaxes of those objects. The lines fitted to the parallax-equivalent width data are…

2005 The Astrophysical Journal
Hipparcos 41
Effect of the H I Lyα Chromospheric Flux Anisotropy on the Total Intensity of the Resonantly Scattered Coronal Radiation
DOI: 10.1086/427903 Bibcode: 2005ApJ...622..737A

Auchère, F.

In modeling of the resonantly scattered solar coronal Lyα line of H I, the intensity of the chromospheric source is often assumed to be uniform. We investigate the validity of this assumption. After establishing a correlation between the H I 121.6 nm and He II 30.4 nm line intensities, we build Carrington maps of the Lyα chromosphere from SOHO EUV…

2005 The Astrophysical Journal
SOHO 41
Solar limb faculae
DOI: 10.1051/0004-6361:20052789 Bibcode: 2005A&A...438.1059H

Hirzberger, J.; Wiehr, E.

We observe solar limb faculae at an unprecedented spatial resolution with the new 1 m Swedish Solar Telescope SST on La Palma. Speckle-reconstructed images are used to study 4475 limb facular grains simultaneously in the 430 nm G-band and the 587.5±1.5 continuum up to only 1'' from the limb (cos θ=0.05). No systematic contrast decrease is found ev…

2005 Astronomy and Astrophysics
SOHO 41
Deconstructing NGC 7130
DOI: 10.1086/425913 Bibcode: 2005ApJ...618..167L

Heckman, T. M.; Levenson, N. A.; Weaver, K. A. +2 more

Observations of the Seyfert 2 and starburst galaxy NGC 7130 with the Chandra X-Ray Observatory illustrate that both of these phenomena contribute significantly to the galaxy's detectable X-ray emission. The active galactic nucleus (AGN) is strongly obscured, buried beneath column density NH>1024cm-2, and it is m…

2005 The Astrophysical Journal
eHST 40
Far Ultraviolet Spectroscopic Explorer Measurements of Interstellar Fluorine
DOI: 10.1086/426778 Bibcode: 2005ApJ...619..884F

Federman, S. R.; Lambert, David L.; Smith, V. V. +1 more

The source of fluorine is not well understood, although core-collapse supernovae, Wolf-Rayet stars, and asymptotic giant branch stars have been suggested. A search for evidence of the ν-process during Type II supernovae is presented. Absorption from interstellar F I is seen in spectra of HD 208440 and HD 209339A acquired with the Far Ultraviolet S…

2005 The Astrophysical Journal
eHST 40
The Ultraviolet Spectrum of η Carinae: Investigation of the Ejecta Absorption
DOI: 10.1086/427437 Bibcode: 2005ApJS..157..138N

Gull, T. R.; Nielsen, K. E.; Vieira Kober, G.

We have investigated the far- through mid-UV (1150-2360 Å) spectrum of η Carinae during the late stages of its broad maximum using the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) moderate dispersion echelle modes. The η Car spectrum is a mixture of absorption and emission lines from the surrounding nebula superimposed …

2005 The Astrophysical Journal Supplement Series
eHST 40
Nonlinear Alfvén, magnetosonic, sound, and electron inertial waves in fluid formalism
DOI: 10.1029/2004JA010852 Bibcode: 2005JGRA..110.3220S

Stasiewicz, K.

A fluid model of nonlinear electron and ion inertial waves in anisotropic plasmas is presented. The model has been verified for plasma beta (ratio of kinetic/magnetic pressures) in a range between 0.1 and 15. It is shown that warm plasmas support four types of nonlinear waves, which correspond to four linear modes, Alfvénic, magnetosonic, sound, a…

2005 Journal of Geophysical Research (Space Physics)
Cluster 40
Metallicities of the β Cephei stars from low-resolution ultraviolet spectra
DOI: 10.1051/0004-6361:20040396 Bibcode: 2005A&A...433..659N

Niemczura, E.; Daszyńska-Daszkiewicz, J.

We derive basic stellar parameters (angular diameters, effective temperatures, metallicities) and interstellar reddening for all β Cephei stars observed during the IUE satellite mission, including those belonging to three open clusters. The parameters are derived by means of an algorithmic procedure of fitting theoretical flux distributions to the…

2005 Astronomy and Astrophysics
IUE 40
On the Afterglow and Host Galaxy of GRB 021004: A Comprehensive Study with the Hubble Space Telescope
DOI: 10.1086/432633 Bibcode: 2005ApJ...633..317F

Pian, E.; Kouveliotou, C.; Tanvir, N. +24 more

We report on Hubble Space Telescope (HST) observations of the late-time afterglow and host galaxy of GRB 021004 (z=2.33). Although this gamma-ray burst (GRB) is one of the best observed so far in terms of sampling in the time domain, multiwavelength coverage, and polarimetric observations, there is substantial disagreement between different interp…

2005 The Astrophysical Journal
eHST 40