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Asiago eclipsing binaries program. III. V570 Persei
DOI: 10.1051/0004-6361:20079305 Bibcode: 2008A&A...483..263T

Munari, U.; Zwitter, T.; Sordo, R. +4 more

The orbit and physical parameters of the previously unsolved double-lined eclipsing binary V570 Per, discovered by the Hipparcos satellite, were derived using high-resolution Echelle spectroscopy and B, V photoelectric photometry. The metallicity from χ2 analysis of the spectra is [ M/H]=+0.02±0.03, and reddening from interstellar NaI a…

2008 Astronomy and Astrophysics
Hipparcos 11
Complexities of a 3-D plasmoid flux rope as shown by an MHD simulation
DOI: 10.1029/2008JA013328 Bibcode: 2008JGRA..11312202F

Baker, D. N.; Wiltberger, M.; Farr, N. L.

The results of a global magnetohydrodynamic (MHD) simulation of a pair of magnetospheric substorms on 11 August 2002 are presented. Comparisons of data with simulation results reveal a good agreement regarding the sequence of events during substorm development. We give particular emphasis to results in the simulation of a flux rope formed during t…

2008 Journal of Geophysical Research (Space Physics)
Cluster 11
Line intensity enhancements in stellar coronal X-ray spectra due to opacity effects
DOI: 10.1051/0004-6361:20079040 Bibcode: 2008A&A...483..887R

Mathioudakis, M.; Keenan, F. P.; Matranga, M. +2 more

Context: The I(15.01 Å)/I(16.78 Å) emission line intensity ratio in Fe xvii has been reported to deviate from its theoretical value in solar and stellar X-ray spectra. This is attributed to opacity in the 15.01 Å line, leading to a reduction in its intensity, and was interpreted in terms of a geometry in which the emitters and absorbers are spatia…

2008 Astronomy and Astrophysics
XMM-Newton 11
An Analysis of the Dust Halo and Extinction toward X Persei
DOI: 10.1086/523700 Bibcode: 2008ApJ...672..984V

Smith, Randall K.; Valencic, Lynne A.

Interstellar dust grain models are not sufficiently constrained by UV extinction curves to allow researchers to distinguish between them. By testing grain models in the X-ray regime and applying elemental abundance constraints, we show to what extent the models can reproduce the observables in these regimes and whether they are capable of doing so…

2008 The Astrophysical Journal
IUE XMM-Newton 11
Phase-dependent X-ray observations of the β Lyrae system. No eclipse in the soft band
DOI: 10.1051/0004-6361:20078871 Bibcode: 2008A&A...477L..37I

Hamann, W. -R.; Oskinova, L. M.; Ignace, R. +2 more

Aims:We report on observations of the eclipsing and interacting binary β Lyrae from the Suzaku X-ray telescope. This system involves an early B star embedded in an optically and geometrically thick disk that is siphoning atmospheric gases from a less massive late B II companion.
Methods: Motivated by an unpublished X-ray spectrum from the Eins…

2008 Astronomy and Astrophysics
Suzaku 11
Discovery of X-ray pulsations from the HMXB source AXJ1749.1-2733
DOI: 10.1111/j.1745-3933.2008.00449.x Bibcode: 2008MNRAS.386L..10K

Tsygankov, S. S.; Lutovinov, A. A.; Karasev, D. I.

We are reporting the discovery of X-ray pulsations from the source AXJ1749.1-2733 with the period of ~132 s based on the XMM-Newton data obtained in 2007 March. The observed pulse profile has a double-peaked structure with the pulse fraction of about 25-30 per cent in the 3-10 keV energy band. We have also found that a periodicity with practically…

2008 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 11
IRAS 04325+2402C: A Very Low Mass Object with an Edge-On Disk
DOI: 10.1086/590339 Bibcode: 2008ApJ...681L..29S

Wood, Kenneth; Doyon, René; Lafrenière, David +3 more

IRAS 04325+2402C is a low-luminosity object located near a protostar in Taurus. We present new spatially resolved millimeter observations, near-infrared spectroscopy, and Spitzer photometry that improve the constraints on the nature of this source. The object is clearly detected in our 1.3 mm interferometry map, allowing us to estimate the mass in…

2008 The Astrophysical Journal
eHST 11
Rosetta target asteroid 2867 Steins: An unusual E-type asteroid
DOI: 10.1111/j.1945-5100.2008.tb01089.x Bibcode: 2008M&PS...43..905W

Weissman, Paul R.; Hicks, Michael D.; Choi, Young-Jun +2 more

ESA's Rosetta spacecraft will fly by main-belt asteroid 2867 Steins on September 5, 2008. We obtained new visible wavelength spectra of 2867 Steins on December 19, 2006 (UT), using the Palomar 5 m telescope and the facility Double Spectrograph. Two sets of spectra, taken ∼3 h apart, one half of the rotation period for 2867 Steins, show it to be an…

2008 Meteoritics and Planetary Science
Rosetta 11
Modified gradiometer technique applied to Double Star (TC-1)
DOI: 10.1016/j.asr.2008.01.014 Bibcode: 2008AdSpR..41.1579G

Zhang, T. L.; Takada, T.; Carr, C. M. +6 more

On TC-1 (Tan Ce 1), the equatorial spacecraft of the Double Star mission, a strong spin-synchronized magnetic interference from the solar panels was observed. In-flight correction techniques for spinning spacecraft that are based on minimizing spin tones in the spin-aligned component and in the magnitude of the ambient magnetic field are therefore…

2008 Advances in Space Research
DoubleStar 11
Medium-latitude sources of plasmaspheric nonthermal continuum radiations observed close to harmonics of the electron gyrofrequency
DOI: 10.1029/2008JA013290 Bibcode: 2008JGRA..11311216G

Grimald, S.; Canu, P.; DéCréAu, P. M. E. +2 more

Nonthermal continuum (NTC) radiation is, with auroral kilometric radiation (AKR), one of the two electromagnetic emissions generated within the Earth's magnetosphere and radiated into space. It is generally believed that NTC is emitted in the plasmapause density gradient after conversion of intense electrostatic waves, present near the magnetic eq…

2008 Journal of Geophysical Research (Space Physics)
Cluster 11