Search Publications

Evidence for a Fast Decline in the Progenitor Population of Gamma-Ray Bursts and the Nature of Their Origin
DOI: 10.1086/342467 Bibcode: 2002ApJ...578..304S

Hurley, K.; Atteia, J. -L.; Stern, B. E.

We show that the source population of long gamma-ray bursts (GRBs) has declined by at least a factor of 12 (at the 90% confidence level) since the early stages of the universe (z~2-3). This result has been obtained using the combined BATSE and Ulysses GRB brightness distribution and the detection of four GRBs with known redshifts brighter than 10<…

2002 The Astrophysical Journal
Ulysses 19
An erupting macrospicule. Characteristics derived from SOHO-CDS spectroscopic observations
DOI: 10.1051/0004-6361:20011819 Bibcode: 2002A&A...384..303P

Bromage, G. E.; Parenti, S.; Bromage, B. J. I.

We report results from the analysis of a sequence of SOHO/CDS observations obtained off-limb in the south polar coronal hole on 6 March 1998. Three successive data sets were obtained with the Normal Incidence Spectrometer (NIS), the first of which showed a jet-like feature visible in the chromospheric and low transition region lines. The morpholog…

2002 Astronomy and Astrophysics
SOHO 19
Linear polarization of the O VI lambda 1031.92 coronal line. I. Constraints on the solar wind velocity field vector in the polar holes
DOI: 10.1051/0004-6361:20020752 Bibcode: 2002A&A...390..691R

Bommier, V.; Raouafi, N. -E.; Lemaire, P. +1 more

In the first part of the present work, we report on the determination of the linear polarization parameters of the O VI lambda1031 .92 coronal line (hereafter O VI D2). Spectropolarimetric observations done by the SUMER spectrometer on board the spacecraft SoHO during minimum activity of the solar cycle (March, 1996) in the south corona…

2002 Astronomy and Astrophysics
SOHO 19
Is TU UMi a W UMa-type system
Bibcode: 2002CoAst.142...57R

Amado, P. J.; Olivares, I.; Rolland, A. +4 more

TU UMi is catalogued as a delta Scuti star, it was discovered by Hipparcos (ESA 1997). Analysis of photometric observations carried through the years 2001 and 2002 is presented. We obtain one only frequency that it is in agreement with it listed in the Hipparcos Catalogue. Using the derived uvbybeta indices, the most relevant physical parameters o…

2002 Communications in Asteroseismology
Hipparcos 19
Resolving the compact H II regions in N160A with HST
DOI: 10.1051/0004-6361:20011577 Bibcode: 2002A&A...381..941H

Schaerer, D.; Heydari-Malayeri, M.; Charmandaris, V. +4 more

Using high-resolution imaging with the Hubble Space Telescope, we study the Large Magellanic Cloud H II region N160A and uncover several striking features of this complex massive star-forming site. The two compact high excitation H II, blobs (HEBs) A1 and A2 are for the first time resolved and their stellar content and morphology is revealed. A1, …

2002 Astronomy and Astrophysics
eHST 19
Subaru optical observations of the old pulsar PSR B0950+08
DOI: 10.1051/0004-6361:20021155 Bibcode: 2002A&A...394..633Z

Kawai, N.; Zharikov, S. V.; Shibanov, Yu. A. +6 more

We report the B band optical observations of an old (tau ~ 17.5 Myr) radiopulsar PSR B0950+08 obtained with the Suprime-Cam at the Subaru telescope. We detected a faint object, B=27fm07 +/-0.16. Within our astrometrical accuracy it coincides with the radio position of the pulsar and with the object detected earlier by Pavlov et al. (\cite{Pavlov})…

2002 Astronomy and Astrophysics
eHST 19
The complete far infrared spectroscopic survey of Herbig AeBe stars obtained by ISO-LWS
DOI: 10.1051/0004-6361:20020977 Bibcode: 2002A&A...395..637L

Benedettini, M.; Elia, D.; Lorenzetti, D. +4 more

The ISO-LWS archive has been systematically searched in order to obtain a complete far IR spectrophotometric survey of Herbig AeBe (HAEBE) stars. The investigated sample is constituted by 15 objects which, together with the 11 HAEBE we have published in two previous papers, represents about 25% of all the known HAEBE. This catalogue constitues an …

2002 Astronomy and Astrophysics
ISO 19
Solar cycle variation of the radiance and the global electron density of the solar corona
DOI: 10.1016/S0273-1177(01)00599-3 Bibcode: 2002AdSpR..29..373L

Llebaria, A.; Quemerais, E.; Lamy, P.

The question of the global activity of the solar corona, as a function of time and distance from the center of the Sun, is considered by analyzing SOHO/LASCO-C2 daily polarized images over four years, i.e., from the minimum to the rising phase of the 23rd solar cycle. After proper correction for instrumental polarization, they are combined to prod…

2002 Advances in Space Research
SOHO 19
Near- and mid-infrared colours of star-forming galaxies in European Large Area ISO Survey fields
DOI: 10.1046/j.1365-8711.2002.06006.x Bibcode: 2002MNRAS.337.1043V

Serjeant, S.; Morel, T.; Gruppioni, C. +6 more

We present J- and K-band near-infrared (near-IR) photometry of a sample of mid-infrared (mid-IR) sources detected by the Infrared Space Observatory (ISO) as part of the European Large Area ISO Survey (ELAIS) and study their classification and star-forming properties. We have used the Preliminary ELAIS Catalogue for the 6.7-µm (LW2) and 15-&m…

2002 Monthly Notices of the Royal Astronomical Society
ISO 19
The charge and velocity detector of the cosmic dust analyzer on Cassini
DOI: 10.1016/S0032-0633(02)00019-3 Bibcode: 2002P&SS...50..773A

Kempf, S.; Srama, R.; Grün, E. +2 more

The cosmic dust analyzer aboard the Cassini spacecraft includes a charge and velocity detector which senses electric charges >10 -15 C of individual cosmic dust grains as they enter the instrument. Charge is an important property of each grain, because it affects its orbital dynamics and is a measure of its size. The duration and sha…

2002 Planetary and Space Science
Cassini 19