Search Publications

Testing the inverse-Compton catastrophe scenario in the intra-day variable blazar S5 0716+71. II. A search for intra-day variability at millimetre wavelengths with the IRAM 30 m telescope
DOI: 10.1051/0004-6361:20054649 Bibcode: 2006A&A...456..117A

Grewing, M.; Britzen, S.; Wagner, S. J. +12 more

We report on a densely time sampled polarimetric flux density monitoring of the BL Lac object S5 0716+71 at 86 GHz and 229 GHz. The source was observed with the IRAM 30 m telescope at Pico Veleta within a coordinated multi-frequency observing campaign, which was centred around a 500 ks INTEGRAL observation during November 10 to …

2006 Astronomy and Astrophysics
INTEGRAL 41
VIMOS-IFU survey of z ~ 0.2 massive galaxy clusters. I. Observations of the strong lensing cluster Abell 2667
DOI: 10.1051/0004-6361:20053384 Bibcode: 2006A&A...456..409C

Kneib, J. -P.; Jullo, E.; Richard, J. +3 more

We present extensive multi-color imaging and low-resolution VIMOS integral field unit (IFU) spectroscopic observations of the X-ray luminous cluster Abell 2667 (z=0.233). An extremely bright giant gravitational arc (z=1.0334 ± 0.0003) is easily identified as part of a triple image system, and other fainter multiple images are also revealed by the …

2006 Astronomy and Astrophysics
eHST 41
Detection of water ice grains after the DEEP IMPACT onto Comet 9P/Tempel 1
DOI: 10.1051/0004-6361:200600003 Bibcode: 2006A&A...448L..53S

Rodriguez-Pascual, P. M.; Schulz, R.; Lumb, D. +3 more

Context: Icy grains in the inner coma of a comet may play an important role in the energy balance and in the production of certain gas coma species. Their existence has therefore been assumed repeatedly to explain a variety of observed phenomena. However, owing to their extremely short life time no evidence for the presence of icy grains had been …

2006 Astronomy and Astrophysics
XMM-Newton 41
Seasonal variations of the martian CO over Hellas as observed by OMEGA/Mars Express
DOI: 10.1051/0004-6361:20065586 Bibcode: 2006A&A...459..265E

Bibring, J. -P.; Gondet, B.; Langevin, Y. +6 more

The OMEGA imaging spectrometer aboard Mars Express has been used to study the evolution of the CO abundance over the Hellas basin, as a function of the seasonal cycle. In spite of significant uncertainties, due to the low intensity of the (2-0) CO band at 2.3 µm, these data allow to search for spatial variations over Hellas, where the surfac…

2006 Astronomy and Astrophysics
MEx 41
Absolute motions of globular clusters. II. HST astrometry and VLT radial velocities in NGC 6397
DOI: 10.1051/0004-6361:20064960 Bibcode: 2006A&A...456..517M

Anderson, J.; Milone, A. P.; Bedin, L. R. +5 more

In this paper we present a new, accurate determination of the three components of the absolute space velocity of the Galactic globular cluster NGC 6397 (l≃338°, b≃-12°). We used three HST/WFPC2 fields with multi-epoch observations to obtain astrometric measurements of objects in three different fields in this cluster. The identification of 33 back…

2006 Astronomy and Astrophysics
eHST 40
Stellar archaeology: the evolving spectrum of FG Sagittae
DOI: 10.1051/0004-6361:20047075 Bibcode: 2006A&A...459..885J

Jeffery, C. S.; Schönberner, D.

Over an interval of 120 years, the extraordinary object FG Sge has been transformed from a hot post-AGB star to a very luminous cool supergiant. Theoretically, this evolution has been associated with the reignition of a helium-shell during the post-AGB stage. A series of studies of the chemical composition of the photosphere hav…

2006 Astronomy and Astrophysics
IUE 40
Multi-wavelength afterglow observations of the high redshift GRB 050730
DOI: 10.1051/0004-6361:20065010 Bibcode: 2006A&A...460..415P

McBreen, S.; Bremer, M.; Tanvir, N. +22 more

Context: .GRB 050730 is a long duration high-redshift burst (z=3.967) that was discovered by Swift. The afterglow shows variability and was well monitored over a wide wavelength range. We present comprehensive temporal and spectral analysis of the afterglow of GRB 050730 including observations covering the wavelength range from the millimeter to X…

2006 Astronomy and Astrophysics
XMM-Newton 40
Dust-scattered X-ray halos around gamma-ray bursts: GRB 031203 revisited and the new case of GRB 050713A
DOI: 10.1051/0004-6361:20054162 Bibcode: 2006A&A...449..203T

Tiengo, A.; Mereghetti, S.

Scattering by interstellar dust grains can produce time variable X-ray halos around gamma-ray bursts (GRB). In particular, an X-ray expanding ring is expected when a short pulse of X-ray radiation is scattered by a narrow layer of dust in our Galaxy. We present a new method for detecting and analyzing dust-scattering expanding rings around gamma-r…

2006 Astronomy and Astrophysics
XMM-Newton 40
On the horizontal branch of the galactic globular cluster NGC 2808
DOI: 10.1051/0004-6361:20042170 Bibcode: 2006A&A...446..569C

Zoccali, M.; Bono, G.; Cassisi, S. +3 more

We present new UV (F218W) data for stars in the central region of the Galactic globular cluster NGC 2808, collected with the WFPC2 camera on board the Hubble Space Telescope. These data together with F439W and F555W-band data and previous ground-based observations provide a multifrequency coverage of the cluster stellar population extending up to …

2006 Astronomy and Astrophysics
eHST 40
Probing the proper motion of the central compact object in Puppis-A with the Chandra high resolution camera
DOI: 10.1051/0004-6361:20065941 Bibcode: 2006A&A...457L..33H

Hui, C. Y.; Becker, W.

By making use of the sub-arcsecond angular resolution of the High Resolution Camera (HRC-I) aboard the Chandra X-ray satellite we have examined the central compact object RX J0822-4300 in the supernova remnant Puppis-A for a possible proper motion. Using data which span an epoch of 1952 days we found the position of RX J0822-4300 different by 0.57…

2006 Astronomy and Astrophysics
XMM-Newton 40