Search Publications

Mira kinematics in the post-Hipparcos era
DOI: 10.1051/0004-6361:20020084 Bibcode: 2002A&A...384..925K

Schilbach, E.; Kharchenko, N.; Malkov, O. +1 more

The complete data set of Mira variables from the 4th edition of the General Catalog of Variable Stars was analyzed and supplemented by the proper motions and radial velocities presently available for Miras. The resulting sample of 724 Miras with periods between 78 and 612 days contains proper motions reduced to the Hipparcos system, radial velocit…

2002 Astronomy and Astrophysics
Hipparcos 14
XMM-Newton observations of MR Vel/RX J0925.7-4758
DOI: 10.1051/0004-6361:20020966 Bibcode: 2002A&A...393..913M

Motch, C.; Neiner, C.; Bearda, H.

We report on XMM-Newton observations of the galactic supersoft X-ray source RX J0925.7-4758 . The RGS spectrum exhibits a wealth of spectral features from iron and oxygen. XMM-Newton data confirm the finding of previous Chandra HETGS/MEG observations that NLTE models of hot white dwarf atmospheres fail to represent the complex s…

2002 Astronomy and Astrophysics
XMM-Newton 14
Stokes parameters of resonance lines scattered by a moving, magnetic medium. Theory of the two-level atom
DOI: 10.1051/0004-6361:20020113 Bibcode: 2002A&A...386..721R

Raouafi, N. -E.

The aim of the present work is to present theoretical results on the Stokes parameters of a resonance spectral line, scattered by moving atoms (or ions) in the presence of a local magnetic field. We assume that the scattered line is sensitive to the Hanle effect due to the magnetic field and also to Doppler redistribution due to the atomic motions…

2002 Astronomy and Astrophysics
SOHO 13
A study of accretion discs around rapidly rotating neutron stars in general relativity and its applications to four low mass X-ray binaries
DOI: 10.1051/0004-6361:20011758 Bibcode: 2002A&A...383..524B

Bhattacharyya, Sudip

We calculate the accretion disc temperature profiles, disc luminosities and boundary layer luminosities for rapidly rotating neutron stars considering the full effect of general relativity. We compare the theoretical values of these quantities with their values inferred from EXOSAT data for four low mass X-ray binary sources: XB 1820-30, GX 17+2, …

2002 Astronomy and Astrophysics
Exosat 13
HD 112 mu m in absorption and extreme CO depletion in a cold molecular cloud
DOI: 10.1051/0004-6361:20020001 Bibcode: 2002A&A...383L...9C

Maret, S.; Ceccarelli, C.; Pagani, L. +3 more

We present ISO-LWS observations at high spectral resolution (R ~ 104) towards a cold molecular cloud in the line of sight of W49. The HD ground state transition at 112 mu m is detected, showing the first observation of this line in absorption outside the solar system. The 112 mu m absorption depth gives a straightforward measure of the …

2002 Astronomy and Astrophysics
ISO 13
The 3-D ionization structure of the planetary nebula NGC 6565
DOI: 10.1051/0004-6361:20020109 Bibcode: 2002A&A...384.1062T

Sabbadin, F.; Turatto, M.; Cappellaro, E. +2 more

A detailed study of the planetary nebula NGC 6565 has been carried out on long-slit echellograms (lambda /Delta lambda =60 000, spectral range = lambda lambda 3900-7750 Å) at six, equally spaced position angles. The expansion velocity field, the c(Hβ ) distribution and the radial profile of the physical conditions (electron temperature and density…

2002 Astronomy and Astrophysics
eHST 13
Multiwavelength evidence for a 15-year periodic activity in the symbiotic nova V1016 Cygni
DOI: 10.1051/0004-6361:20020847 Bibcode: 2002A&A...391..999P

Chochol, D.; Buson, L. M.; Vittone, A. A. +2 more

The ~ 15.1 years period found in the long-term UBV photoelectric and photographic photometry of the symbiotic nova V1016 Cyg is detected also in the (J-K) colour index and in the UV continuum and emission line fluxes from IUE and HUT spectra. It could be interpreted either as the effect of recurrent enhanced mass loss episodes from the Mira type v…

2002 Astronomy and Astrophysics
IUE 13
Asteroids observations with the Hubble Space Telescope. I. Observing strategy, and data analysis and modeling process
DOI: 10.1051/0004-6361:20020873 Bibcode: 2002A&A...391.1123H

Lattanzi, M.; Tanga, P.; Berthier, J. +5 more

Five main belt asteroids and one Trojan - selected mainly on the basis of their possible binary nature as deduced from light curve morphology - have been observed with the Fine Guidance Sensors (FGS#3 and FGSR#1) of the Hubble Space Telescope (HST). In this first paper we present the selection and observation strategy, data reduction and analysis.…

2002 Astronomy and Astrophysics
eHST 13
Search for duplicity in periodic variable Be stars
DOI: 10.1051/0004-6361:20020174 Bibcode: 2002A&A...385..488C

Carrier, F.; Burki, G.; Burnet, M.

Four Be stars, HR 1960, HR 2968, HR 3237 and HR 3642, selected according to their periodic variations in HIPPARCOS and GENEVA photometries, were monitored from 1998 until 2001 with the CORALIE spectrograph. Among these stars, two are new spectroscopic binaries and one is a…

2002 Astronomy and Astrophysics
Hipparcos 13
On the theory of MAG waves and a comparison with sunspot observations from CDS/SoHO
DOI: 10.1051/0004-6361:20021257 Bibcode: 2002A&A...395..263B

Doyle, J. G.; Poedts, S.; Banerjee, D. +2 more

We examine the influence of non-adiabatic effects on the modes of an isothermal stratified magnetic atmosphere. We present new solutions for magneto-acoustic-gravity (or MAG) waves in the presence of a radiative heat exchange based on Newton's law of cooling. An analytic expression for the dispersion relation is derived, which allows the effect of…

2002 Astronomy and Astrophysics
SOHO 13