Search Publications

First albedo determination of 2867 Steins, target of the Rosetta mission
DOI: 10.1051/0004-6361:20064913 Bibcode: 2006A&A...449L...9F

Barbieri, C.; Barucci, M. A.; Fornasier, S. +2 more

Aims. We present the first albedo determination of 2867 Steins, the asteroid target of the Rosetta space mission together with 21 Lutetia.Methods.The data were obtained in polarimetric mode at the ESO-VLT telescope with the FORS1 instrument in the V and R filters. Observations were carried out from June to August 2005 covering the phase angle rang…

2006 Astronomy and Astrophysics
Rosetta 32
A self-consistent model of isolated neutron stars: the case of the X-ray pulsar RX J0720.4-3125
DOI: 10.1051/0004-6361:20065827 Bibcode: 2006A&A...459..175P

Miniutti, G.; Pons, J. A.; Pérez-Azorín, J. F. +1 more

Context: .We present a unified explanation for the observed properties of the isolated neutron star RX J0720.4-3125 by obtaining a self-consistent model that accounts simultaneously for the observed X-ray spectrum and optical excess, the pulsed fraction, the observed spectral feature around 0.3 keV, and the long-term spectral evolution.
Aims: …

2006 Astronomy and Astrophysics
XMM-Newton 32
X-rays from HH 210 in the Orion nebula
DOI: 10.1051/0004-6361:200600004 Bibcode: 2006A&A...448L..29G

Grosso, N.; Kastner, J. H.; Bally, J. +3 more

We report the detection during the Chandra Orion Ultradeep Project (COUP) of two soft, constant, and faint X-ray sources associated with the Herbig-Haro object HH 210. HH 210 is located at the tip of the NNE finger of the emission line system bursting out of the BN-KL complex, northwest of the Trapezium cluster in the OMC-1 molecular cloud. Using …

2006 Astronomy and Astrophysics
eHST 31
INTEGRAL observations of the Crab pulsar
DOI: 10.1051/0004-6361:20054305 Bibcode: 2006A&A...450..617M

Cusumano, G.; Foschini, L.; Di Cocco, G. +5 more

Aims.The paper presents the timing and spectral analysis of several observations of the Crab pulsar performed with INTEGRAL in the energy range 3-500 keV.
Methods: .All these observations, when summed together provide a high statistics data set which can be used for accurate phase resolved spectroscopy. A detailed study of …

2006 Astronomy and Astrophysics
INTEGRAL 31
X-ray emission from the blazar AO 0235+16: the XMM-Newton and Chandra point of view
DOI: 10.1051/0004-6361:20054409 Bibcode: 2006A&A...452..845R

Villata, M.; Orio, M.; Raiteri, C. M. +4 more

We analyse five observations of the BL Lac object AO 0235+16 performed with the Chandra and XMM-Newton satellites during the years 2000-2005. In the February 2002 observation the source is found in a bright state and presents a steep X-ray spectrum, while in all the other epochs it is faint and the spectrum is hard. The soft X-r…

2006 Astronomy and Astrophysics
XMM-Newton 31
Observation of a bright coronal downflow by SOHO/EIT
DOI: 10.1051/0004-6361:20053840 Bibcode: 2006A&A...449..369T

Solanki, S. K.; Schwenn, R.; Mierla, M. +3 more

A distinct coronal downflow has been discovered in the course of a prominence eruption associated coronal mass ejection (CME) imaged by EIT (Extreme ultraviolet Imaging Telescope) and LASCO (Large Angle Spectrometric Coronagraph) on board SOHO (Solar and Heliospheric Observatory) on 5-Mar.-2000. Evolution of the prominences seen by EIT was tracked…

2006 Astronomy and Astrophysics
SOHO 30
Tests of stellar model atmospheres by optical interferometry. IV. VINCI interferometry and UVES spectroscopy of Menkar
DOI: 10.1051/0004-6361:20066032 Bibcode: 2006A&A...460..855W

Wolff, B.; Driebe, T.; Wittkowski, M. +3 more

Aims.We present coordinated near-infrared K-band interferometric and optical spectroscopic observations of the M 1.5 giant α Cet (Menkar) obtained with the instruments VINCI and UVES at the Paranal Observatory. Spherically symmetric PHOENIX stellar model atmospheres are constrained by comparison to our interferometric and spectr…

2006 Astronomy and Astrophysics
Hipparcos 30
The X-ray binary 2S0114+650=LSI+65 010. A slow pulsar or tidally-induced pulsations?
DOI: 10.1051/0004-6361:20065305 Bibcode: 2006A&A...458..513K

Koenigsberger, G.; Canalizo, G.; Richer, M. G. +4 more

Context: .The X-ray source 2S0114+650=LSI+65 010 is a binary system containing a B-type primary and a low mass companion believed to be a neutron star. The system has three reported periodicities: the orbital period, P_orb∼11.6 days, X-ray flaring with P_flare∼2.7 h and a "superorbital" X-ray periodicity P_super=30.7 days.
Aims: .The objective…

2006 Astronomy and Astrophysics
INTEGRAL 30
A historic jet-emission minimum reveals hidden spectral features in 3C 273
DOI: 10.1051/0004-6361:200600023 Bibcode: 2006A&A...451L...1T

Lähteenmäki, A.; Foellmi, C.; O'Brien, P. T. +14 more

Aims. The aim of this work is to identify and study spectral features in the quasar 3C 273 usually blended by its strong jet emission.
Methods: . A historic minimum in the sub-millimetre emission of 3C 273 triggered coordinated multi-wavelength observations in June 2004. X-ray observations from the INTEGRAL, XMM-Newton and RXTE satellites are…

2006 Astronomy and Astrophysics
INTEGRAL XMM-Newton 30
New southern blue compact dwarf galaxies in the 2dF Galaxy redshift survey
DOI: 10.1051/0004-6361:20054458 Bibcode: 2006A&A...457...45P

Thuan, T. X.; Izotov, Y. I.; Papaderos, P. +3 more

Aims.Aiming to find new extremely metal-deficient star-forming galaxies we extracted from the Two-Degree Field Galaxy Redshift Survey (2dFGRS) 100 K Data Release 14 emission-line galaxies with relatively strong [O iii] λ4363 emission.
Methods: .Spectroscopic and photometric studies of this sample and, in addition, of 7 Tololo and 2 UM galaxies…

2006 Astronomy and Astrophysics
eHST 30