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Photometric properties of the Local Volume dwarf galaxies
DOI: 10.1111/j.1365-2966.2007.12814.x Bibcode: 2008MNRAS.384.1544S

Dolphin, A. E.; Tully, R. Brent; Sharina, M. E. +9 more

We present surface photometry and metallicity measurements for 104 nearby dwarf galaxies imaged with the Advanced Camera for Surveys and Wide Field and Planetary Camera 2 aboard the Hubble Space Telescope. In addition, we carried out photometry for 26 galaxies of the sample and for Sextans B on images of the Sloan Digital Sky Survey. Our sample co…

2008 Monthly Notices of the Royal Astronomical Society
eHST 63
Detection of a Hot Subdwarf Companion to the Be Star FY Canis Majoris
DOI: 10.1086/591145 Bibcode: 2008ApJ...686.1280P

Gies, Douglas R.; Peters, Geraldine J.; Grundstrom, Erika D. +1 more

The rapid rotation of Be stars may be caused in some cases by past mass and angular momentum accretion in an interacting binary in which the mass donor is currently viewed as a small, hot subdwarf stripped of its outer envelope. Here we report on the spectroscopic detection of such a subdwarf in the Be binary system FY Canis Majoris from the analy…

2008 The Astrophysical Journal
IUE 63
Phyllosilicate and sulfate-hematite deposits within Miyamoto crater in southern Sinus Meridiani, Mars
DOI: 10.1029/2008GL035363 Bibcode: 2008GeoRL..3519204W

Clark, R. N.; Arvidson, R. E.; Morris, R. V. +13 more

Orbital topographic, image, and spectral data show that sulfate- and hematite-bearing plains deposits similar to those explored by the MER rover Opportunity unconformably overlie the northeastern portion of the 160 km in diameter Miyamoto crater. Crater floor materials exhumed to the west of the contact exhibit CRISM and OMEGA NIR spectral signatu…

2008 Geophysical Research Letters
MEx 63
Unresolved emission and ionized gas in the bulge of M31
DOI: 10.1111/j.1365-2966.2008.13391.x Bibcode: 2008MNRAS.388...56B

Bogdán, Á.; Gilfanov, M.

We study the origin of unresolved X-ray emission from the bulge of M31 based on archival Chandra and XMM-Newton observations. We demonstrate that three different components are present. (i) Broad-band emission from a large number of faint sources - mainly accreting white dwarfs and active binaries, associated with the old stellar population, simil…

2008 Monthly Notices of the Royal Astronomical Society
XMM-Newton 63
Magnetic fields and gas in the cluster-influenced spiral galaxy NGC 4254. II. Structures of magnetic fields
DOI: 10.1051/0004-6361:20078688 Bibcode: 2008A&A...482..755C

Chyży, K. T.

Aims: The origin of asymmetric radio polarized emission in the Virgo Cluster spiral NGC 4254 is investigated and the influence of cluster environment on the properties of magnetic fields is explored.
Methods: Structures of magnetic fields are analyzed with the concept of “magnetic maps”, presenting distributions of different magnetic field com…

2008 Astronomy and Astrophysics
XMM-Newton 63
Hard X-ray emission from η Carinae
DOI: 10.1051/0004-6361:20078981 Bibcode: 2008A&A...477L..29L

Walter, R.; Rauw, G.; Leyder, J. -C.

Context: If relativistic particle acceleration takes place in colliding-wind binaries, hard X-rays and γ-rays are expected through inverse Compton emission, but to date these have never been unambiguously detected.
Aims: To detect this emission, observations of η Carinae were performed with INTEGRAL, leveraging its high spat…

2008 Astronomy and Astrophysics
INTEGRAL 63
Cluster observations of the Earth's quasi-parallel bow shock
DOI: 10.1029/2007JA012756 Bibcode: 2008JGRA..113.7S02L

Dandouras, I.; RèMe, H.; Horbury, T. S. +1 more

Cluster observations of the Earth's quasi-parallel shock are used to investigate properties of the transition and the role of magnetic pulsations in the shock process. We use crossings at small spacecraft separations to show that pulsations grow in only a few seconds. We then use an example when the spacecraft were only a few thousand kilometers a…

2008 Journal of Geophysical Research (Space Physics)
Cluster 63
A new view of quiet-Sun topology from Hinode/SOT
DOI: 10.1051/0004-6361:200809826 Bibcode: 2008A&A...484L..47R

Régnier, S.; Parnell, C. E.; Haynes, A. L.

Context: With the recent launch of the Hinode satellite our view of the nature and evolution of quiet-Sun regions has been improved. In light of the new high resolution observations, we revisit the study of the quiet Sun's topological nature.
Aims: Topology is a tool to explain the complexity of the magnetic field, the occurrence of reconnecti…

2008 Astronomy and Astrophysics
Hinode 63
High-resolution optical spectroscopy of Plaskett's star
DOI: 10.1051/0004-6361:200810003 Bibcode: 2008A&A...489..713L

Martins, F.; Gosset, E.; Rauw, G. +3 more

Context: Plaskett's star (HD 47 129) is a very massive O + O binary that belongs to the Mon OB2 association. Previous work suggests that this system displays the Struve-Sahade effect although the measurements of the secondary radial velocities are very difficult and give controversial results. Both components have powerful stell…

2008 Astronomy and Astrophysics
IUE 63
Characteristics of middle- to low-latitude Pi2 excited by bursty bulk flows
DOI: 10.1029/2007JA012629 Bibcode: 2008JGRA..113.7S15C

Zong, Qiugang; Lucek, E.; Zhang, Tielong +13 more

This paper, by using the data of Cluster, TC-1, GOES, and eight ground stations on 22 October 2004, studied the characteristics of low-latitude Pi2s generated by an earthward bursty bulk flow (BBF) in the near-Earth tail plasma sheet. The BBF excited simultaneously two distinct classes of Pi2s: one is long-period Pi2 (90-130 s) and the other is sh…

2008 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 63