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Chandra and Spitzer observations of CDFS X-ray obscured QSOs
DOI: 10.1051/0004-6361:20065096 Bibcode: 2007A&A...466..823G

Georgakakis, A.; Georgantopoulos, I.; Akylas, A.

We present Chandra and Spitzer data for the 186, extragalactic, hard 2-10 keV X-ray selected sources, which lie in the central part of the Chandra Deep Field South (CDFS). For the vast majority of sources (99.5%), there is a spectroscopic or photometric redshift available. We classify 17 sources as X-ray obscured QSOs, strictly according to X-ray …

2007 Astronomy and Astrophysics
eHST 28
A Galaxy in Transition: Structure, Globular Clusters, and Distance of the Star-Forming S0 Galaxy NGC 1533 in Dorado
DOI: 10.1086/523640 Bibcode: 2007ApJ...671.1624D

Meurer, Gerhardt R.; Blakeslee, John P.; Putman, Mary E. +1 more

We use two-band imaging data from the Advanced Camera for Surveys onboard the Hubble Space Telescope for a detailed study of NGC 1533, an SB0 galaxy in the Dorado group surrounded by a ring of H I. NGC 1533 appears to be completing a transition from late to early type: it is red, but not quite dead. Faint spiral structure becomes visible following…

2007 The Astrophysical Journal
eHST 28
The HeII Fowler lines and the OIII and NIII Bowen fluorescence lines in the symbiotic nova RR Telescopii
DOI: 10.1051/0004-6361:20066175 Bibcode: 2007A&A...464..715S

Danziger, J.; Bonifacio, P.; Selvelli, P.

Aims:A detailed study of the O III and N III Bowen lines in the spectrum of RR Tel.
Methods: Absolute intensities for the He II, O III, and N III emission lines have been obtained from STIS, UVES, FEROS and IUE data, after re-calibration of UVES and FEROS on the STIS scale.
Results: A new measure of reddening (E(B-V) 0.00) has b…

2007 Astronomy and Astrophysics
IUE eHST 28
GQ Lup B Visible and Near-Infrared Photometric Analysis
DOI: 10.1086/511071 Bibcode: 2007ApJ...654L.151M

Macintosh, Bruce; Barman, Travis; Marois, Christian

We have reanalyzed archival HST and Subaru data of the recently discovered planetary mass companion (PMC) GQ Lup B. With these we produce the first R- and I-band photometry of the companion and fit a radius and effective temperature using detailed model atmospheres. We find an effective temperature of 2335+/-100 K, a radius of 0.38+/-0.05 Rso…

2007 The Astrophysical Journal
eHST 28
On the origin of perennial water ice at the south pole of Mars: A precession-controlled mechanism?
DOI: 10.1029/2007JE002902 Bibcode: 2007JGRE..112.8S17M

Bibring, J. -P.; Langevin, Y.; Clancy, R. T. +3 more

The poles of Mars are known to have recorded recent (<107 years) climatic changes. While the south polar region appears to have preserved its million-year-old environment from major resurfacing events, except for the small portion containing the CO2 residual cap, the discovery of residual water ice units in areas adjacent …

2007 Journal of Geophysical Research (Planets)
MEx 28
Photospheric magnetic evolution of super active regions
DOI: 10.1051/0004-6361:20078110 Bibcode: 2007A&A...474..633R

Romano, P.; Zuccarello, F.

Context: Solar flares are one of the most interesting phenomena of solar activity. Although many authors agree that their energy release is related to magnetic reconnection, the phases preceding the magnetic reconnection process are still unclear in several respects.
Aims: We studied the magnetic flux evolution in 26 super active regions obser…

2007 Astronomy and Astrophysics
SOHO 28
The Merger in Abell 576: A Line-of-Sight Bullet Cluster?
DOI: 10.1086/520708 Bibcode: 2007ApJ...668..781D

Bregman, Joel N.; Dupke, Renato A.; Mirabal, Nestor +1 more

Using a combination of Chandra and XMM-Newton observations, we confirmed the presence of a significant velocity gradient along the northeast-southwest direction in the intracluster gas of the cluster Abell 576. The results are consistent with a previous ASCA SIS analysis of this cluster. The error-weighted average over the ACIS-S3 and EPIC MOS1 an…

2007 The Astrophysical Journal
XMM-Newton 28
Initial Observations of Sunspot Oscillations Excited by Solar Flare
DOI: 10.1086/524298 Bibcode: 2007ApJ...670L.147K

Kosovichev, A. G.; Sekii, T.

Observations of a large solar flare on 2006 December 13 using Solar Optical Telescope (SOT) on board the Hinode spacecraft revealed high-frequency oscillations excited by the flare in the sunspot chromosphere. These oscillations are observed in the region of strong magnetic field of the sunspot umbra and may provide a new diagnostic tool for probi…

2007 The Astrophysical Journal
Hinode 28
A study of the Sunyaev-Zel'dovich increment using archival SCUBA data
DOI: 10.1111/j.1365-2966.2007.11443.x Bibcode: 2007MNRAS.376.1073Z

Halpern, Mark; Scott, Douglas; Zemcov, Michael +2 more

In a search for evidence of the short wavelength increment in the Sunyaev-Zel'dovich (SZ) effect, we have analysed archival galaxy cluster data from the Submillimetre Common User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope, resulting in the most complete pointed survey of clusters at 850µm to date. SCUBA's 850-µm passb…

2007 Monthly Notices of the Royal Astronomical Society
XMM-Newton 28
On the distance of PG 1553+11. A lineless BL Lacertae object active in the TeV band
DOI: 10.1051/0004-6361:20078290 Bibcode: 2007A&A...473L..17T

Falomo, R.; Uslenghi, M.; Treves, A.

Context: The redshift of PG 1553+11, a bright BL Lac object (V∼14), is still unknown. It has been recently observed in the TeV band, a fact that offers an upper limit for the redshift z<0.4.
Aims: We intend to provide a lower limit for the distance of the object.
Methods: We used a χ2 procedure to constrain…

2007 Astronomy and Astrophysics
eHST 28