Search Publications

Cassiopeia A dust composition and heating
DOI: 10.1051/0004-6361:20010053 Bibcode: 2001A&A...369..589D

Pantin, E.; Lagage, P. O.; Douvion, T.

Material ejected by a supernova is directly observed in the form of Fast Moving Knots (FMK's) in the Cassiopeia A supernova remnant. Part of this material has condensed into dust. In this paper, by fitting the ISO mid-infrared emission of the dust, we derive the dust composition and discuss the dust heating. The dust is found to be made mainly of …

2001 Astronomy and Astrophysics
ISO 45
Wind circulation in selected rotating magnetic early-B stars
DOI: 10.1051/0004-6361:20010472 Bibcode: 2001A&A...372..208S

Smith, M. A.; Groote, D.

The rotating magnetic B stars are a class of variables consisting of He-strong and some beta Cep stars which have oblique dipolar magnetic fields. Such stars develop co-rotating, torus-shaped clouds by channeling wind particles from their magnetic poles to circumstellar regions centered around the plane of their magnetic equators. The rotation of …

2001 Astronomy and Astrophysics
IUE 45
Reprocessing the Hipparcos data for evolved giant stars II. Absolute magnitudes for the R-type carbon stars
DOI: 10.1051/0004-6361:20010348 Bibcode: 2001A&A...371..222K

Jorissen, A.; Pourbaix, D.; Knapp, G.

The Hipparcos Intermediate Astrometric Data for carbon stars have been reprocessed using an algorithm which provides an objective criterion for rejecting anomalous data points and constrains the parallax to be positive. New parallax solutions have been derived for 317 cool carbon stars, mostly of types R and N. In this paper we discuss the results…

2001 Astronomy and Astrophysics
Hipparcos 45
A Search for Signatures of Quasar Evolution: Comparison of the Shapes of the Rest-Frame Optical/Ultraviolet Continua of Quasars at z>3 and z~0.1
DOI: 10.1086/322535 Bibcode: 2001ApJS..136..225K

Elvis, Martin; Bechtold, Jill; Elston, Richard +1 more

For 15 bright (V<17.5), high-redshift (z>3) quasars, we have obtained infrared spectra and photometry, and optical spectrophotometry and photometry, which we use to construct their spectral energy distributions (SEDs) from λrest~1285-5100 Å. High-resolution spectroscopy for seven enable measurements of their continua shortward of …

2001 The Astrophysical Journal Supplement Series
IUE 45
Cluster magnetic field observations of the bowshock: Orientation, motion and structure
DOI: 10.5194/angeo-19-1399-2001 Bibcode: 2001AnGeo..19.1399H

Balogh, A.; Horbury, T. S.; Lucek, E. A. +7 more

Four spacecraft Cluster magnetic field observations of the low <beta> quasi-perpendicular terrestrial bowshock are presented for the first time. Multiple quasi-perpendicular crossings on 25 December 2000 are analysed. By combining data from the four spacecraft, bowshock orientations and velocities can be calculated. It is shown that, even wh…

2001 Annales Geophysicae
Cluster 45
The X-Ray Afterglow of GRB 000926 Observed by BeppoSAX and Chandra: A Mildly Collimated Fireball in a Dense Medium?
DOI: 10.1086/322467 Bibcode: 2001ApJ...558..442P

Piro, L.; Antonelli, L. A.; Frail, D. A. +8 more

We present X-ray observations of the afterglow of GRB 000926, performed around and after the break observed in the optical light curve 2 days after the burst. The steep X-ray light curve observed around the break confirms the presence of this feature in X-rays. However, the spectral and temporal properties are not consistent with a standard jet sc…

2001 The Astrophysical Journal
Ulysses 44
Infrared spectrum and proper motion of the brown dwarf companion of HR 7329 in Tucanae
DOI: 10.1051/0004-6361:20000051 Bibcode: 2001A&A...365..514G

Neuhäuser, R.; Guenther, E. W.; Huélamo, N. +2 more

Up to now only four brown dwarf companions to normal stars have been found and confirmed by both spectroscopy and proper motion (namely Gl 229 B, G 196-3 B, Gl 570 D, and CoD-33 deg 7795 B). On the basis of an optical spectrum taken with HST/STIS Lowrance et al. (2000) recently po…

2001 Astronomy and Astrophysics
eHST 44
Broadband infrared photometry of comet Hale-Bopp with ISOPHOT
DOI: 10.1051/0004-6361:20011139 Bibcode: 2001A&A...377.1098G

Krüger, H.; Lamy, P.; Keller, H. U. +21 more

Comet Hale-Bopp was observed five times with ISOPHOT, the photometer on board ESA's Infrared Space Observatory (ISO) between 4.6 and 2.8 AU. Each time, broadband photometry was performed using 4 different detectors, 5 apertures and 10 filters covering the range between 3.6 and 170 mu m. Background observations were performed with identical instrum…

2001 Astronomy and Astrophysics
ISO 44
Water in K and M giant stars unveiled by ISO
DOI: 10.1051/0004-6361:20011012 Bibcode: 2001A&A...376L...1T

Tsuji, T.

Based on the spectra obtained with Infrared Space Observatory, ISO, we detected the 6.3 mu m bands of water in the late K giant Aldebaran (alpha Tau) and several early M giant stars (between M0 and M3.5), which have been deemed to be too warm for tri-atomic H2O molecule to reside in their photospheres. The water column densities range (…

2001 Astronomy and Astrophysics
ISO 44
SCUBA photometry of candidate Vega-like sources
DOI: 10.1046/j.1365-8711.2001.04672.x Bibcode: 2001MNRAS.327..133S

Barlow, M. J.; Sylvester, R. J.; Dunkin, S. K.

New SCUBA measurements at millimetre wavelengths are presented for a sample of Vega-like stars. Six stars were detected, while sensitive upper limits were obtained for a further 11 sources. Most of the sample selected from a recent catalogue of Vega-like stars have infrared excesses similar to those of the prototype Vega-like stars α Lyr and α PsA…

2001 Monthly Notices of the Royal Astronomical Society
Hipparcos 44