Search Publications

XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
DOI: 10.1051/0004-6361:20065678 Bibcode: 2006A&A...459..353W

Böhringer, H.; Simionescu, A.; Kaastra, J. S. +3 more

We present a study of chemical abundances in the giant elliptical galaxy M 87 using high-resolution spectra obtained with the Reflection Grating Spectrometers during two deep XMM-Newton observations. While we confirm the two-temperature structure of the inter-stellar medium (ISM) in M 87, we also show that a continuous temperature distribution des…

2006 Astronomy and Astrophysics
XMM-Newton 61
Multifrequency VLBA monitoring of 3C 273 during the INTEGRAL Campaign in 2003. I. Kinematics of the parsec scale jet from 43 GHz data
DOI: 10.1051/0004-6361:20053753 Bibcode: 2006A&A...446...71S

Tornikoski, M.; Wiik, K.; Savolainen, T. +1 more

In this first of a series of papers describing polarimetric multifrequency Very Long Baseline Array (VLBA) monitoring of 3C 273 during a simultaneous campaign with the INTEGRAL γ-ray satellite in 2003, we present 5 Stokes I images and source models at 7 mm. We show that a part of the inner jet (1-2 milliarcsec from the core) is …

2006 Astronomy and Astrophysics
INTEGRAL 61
Hubble Space Telescope observations of the nucleus and inner coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361:20065253 Bibcode: 2006A&A...458..669L

Jorda, L.; Lamy, P. L.; Gutiérrez, P. J. +3 more

Context: .Following the postponement of the launch of the Rosetta spacecraft scheduled in January 2003, comet 67P/Churyumov-Gerasimenko emerged as the most suitable new target. However a critical issue was the size, that is, the mass of its nucleus, as the surface module Philae was designed to land on a nucleus with a radius no larger than approxi…

2006 Astronomy and Astrophysics
Rosetta eHST 60
A hard X-ray view of giga-hertz peaked spectrum radio galaxies
DOI: 10.1051/0004-6361:20053374 Bibcode: 2006A&A...446...87G

Guainazzi, M.; Piconcelli, E.; Grandi, P. +3 more

We present the first broadband X-ray observations of four Giga-Hertz Peaked Spectrum (GPS) radio galaxies at redshift ⪉1 performed by Chandra and XMM-Newton. These observations more than double the number of members of this class with measured spectra in hard (E > 2 keV) X-rays. All sources were detected. Their radio-to-X-ray spectral energy di…

2006 Astronomy and Astrophysics
XMM-Newton 59
Unveiling the nature of INTEGRAL objects through optical spectroscopy. IV. A study of six new hard X-ray sources
DOI: 10.1051/0004-6361:20065111 Bibcode: 2006A&A...455...11M

Palazzi, E.; Masetti, N.; Walter, R. +9 more

We present further results from our onging optical spectrophotometric campaign at the Astronomical Observatory of Bologna in Loiano (Italy) on unidentified hard X-ray sources detected by INTEGRAL. We observed spectroscopically the putative optical counterparts of the INTEGRAL sources IGR J00234+6141, IGR J01583+6713, IGR J06074+2205, IGR J13091+11…

2006 Astronomy and Astrophysics
INTEGRAL 59
XMM-Newton X-ray spectroscopy of classical T Tauri stars
DOI: 10.1051/0004-6361:20054247 Bibcode: 2006A&A...449..737R

Schmitt, J. H. M. M.; Robrade, J.

We present results from a comparative study of XMM-Newton observations of four classical T Tauri stars (CTTS), namely BP Tau, CR Cha, SU Aur and TW Hya. In these objects coronal, i.e. magnetic, activity and as recently shown, magnetically funneled accretion are the process…

2006 Astronomy and Astrophysics
XMM-Newton 58
Simultaneous optical and X-ray observations of a giant flare on the ultracool dwarf LP 412-31
DOI: 10.1051/0004-6361:20066488 Bibcode: 2006A&A...460L..35S

Liefke, C.; Schmitt, J. H. M. M.; Micela, G. +1 more

Cool stars are known to produce flares probably as a result of the magnetic reconnection in their outer atmospheres. We present simultaneous XMM-Newton optical V band and X-ray observations of the M8 dwarf LP 412-31. During the observation a giant flare occurred, with an optical amplitude of 6 mag and total energy of 3 × 1032 erg in bot…

2006 Astronomy and Astrophysics
XMM-Newton 58
Amorphous alumina in the extended atmosphere of α Orionis
DOI: 10.1051/0004-6361:20053359 Bibcode: 2006A&A...447..311V

Waters, L. B. F. M.; Eriksson, K.; Hony, S. +7 more

In this paper we study the extended atmosphere of the late-type supergiant α Orionis. Infrared spectroscopy of red supergiants reveals strong molecular bands, some of which do not originate in the photosphere but in a cooler layer of molecular material above it. Lately, these layers have been spatially resolved by near and mid-IR interferometry. I…

2006 Astronomy and Astrophysics
ISO 57
COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses. II. SDSS J0924+0219: the redshift of the lensing galaxy, the quasar spectral variability and the Einstein rings
DOI: 10.1051/0004-6361:20054423 Bibcode: 2006A&A...451..747E

Magain, P.; Dye, S.; Meylan, G. +4 more

Aims.To provide the observational constraints required to use the gravitationally lensed quasar SDSS J0924+0219 for the determination of H0 from the time delay method. We measure here the redshift of the lensing galaxy, we show the spectral variability of the source, and we resolve the lensed host galaxy of the source.
Methods.We pr…

2006 Astronomy and Astrophysics
eHST 57
Resolving the compact dusty discs around binary post-AGB stars using N-band interferometry
DOI: 10.1051/0004-6361:20054300 Bibcode: 2006A&A...450..181D

Waters, L. B. F. M.; Jaffe, W.; Paresce, F. +8 more

We present the first mid-IR long baseline interferometric observations of the circumstellar matter around binary post-AGB stars. Two objects, SX Cen and HD 52961, were observed using the VLTI/MIDI instrument during Science Demonstration Time. Both objects are known binaries for which a stable circumbinary disc…

2006 Astronomy and Astrophysics
IUE 56