Search Publications

Observation of GRB 030131 with the INTEGRAL satellite
DOI: 10.1051/0004-6361:20031128 Bibcode: 2003A&A...409..831G

Pian, E.; Frontera, F.; Hurley, K. +13 more

A long Gamma-Ray Burst (GRB) was detected with the instruments on board the INTEGRAL satellite on January 31 2003. Although most of the GRB, which lasted ~ 150 s, occurred during a satellite slew, the automatic software of the INTEGRAL Burst Alert System was able to detect it in near-real time. Here we report the results obtained with the IBIS ins…

2003 Astronomy and Astrophysics
INTEGRAL 14
Hyades dynamics from N-body simulations: Accuracy of astrometric radial velocities from Hipparcos
DOI: 10.1051/0004-6361:20030147 Bibcode: 2003A&A...401..565M

Madsen, Søren

The internal velocity structure in the Hyades cluster as seen by Hipparcos is compared with realistic N-body simulations using the NBODY6 code, which includes binary interaction, stellar evolution and the Galactic tidal field. The model allows to estimate reliably the accuracy of astrometric radial velocities in the Hyades as derived by Lindegren …

2003 Astronomy and Astrophysics
Hipparcos 14
New Identifications of Mn VI and Fe VII Vacuum Ultraviolet Lines
DOI: 10.1086/377438 Bibcode: 2003ApJS..148..567E

Feldman, U.; Ekberg, J. O.

The Solar Ultraviolet Measurements of Emitted Radiation (SUMER) spectrometer aboard the Solar and Heliospheric Observatory (SOHO) recorded a large number of spectra in the 500-1600 Å region. Although many of the detected lines have already been identified, the origins of a substantial fraction of the lines remain unknown. In this paper we report o…

2003 The Astrophysical Journal Supplement Series
SOHO 14
Polar, Cluster and SuperDARN evidence for high-latitude merging during southward IMF: temporal/spatial evolution
DOI: 10.5194/angeo-21-2233-2003 Bibcode: 2003AnGeo..21.2233M

Wild, J. A.; Lester, M.; Dunlop, M. +5 more

Magnetic merging on the dayside magnetopause often occurs at high latitudes. Polar measured fluxes of accelerated ions and wave Poynting vectors while skimming the subsolar magnetopause. The measurements indicate that their source was located to the north of the spacecraft, well removed from expected component merging sites. This represents the fi…

2003 Annales Geophysicae
Cluster 14
Emission-Line Galaxies in the Space Telescope Imaging Spectrograph Parallel Survey. I. Observations and Data Analysis
DOI: 10.1086/373988 Bibcode: 2003ApJS..146..209T

Gardner, Jonathan P.; Teplitz, Harry I.; Rhodes, Jason +5 more

In the first 3 years of operation the Space Telescope Imaging Spectrograph (STIS) obtained slitless spectra of ~2500 fields in parallel to prime Hubble Space Telescope (HST) observations as part of the STIS parallel survey (SPS). The archive contains ~300 fields at high Galactic latitude (b>30deg) with spectroscopic exposure times gr…

2003 The Astrophysical Journal Supplement Series
eHST 14
Propagation velocities of gas rings in collisional ring galaxies
DOI: 10.1051/0004-6361:20021910 Bibcode: 2003A&A...400...81V

Bizyaev, D.; Vorobyov, E. I.

The propagation velocity of the first gas ring in collisional ring galaxies, i.e. the velocity at which the maximum in the radial gas density profile propagates radially in the galactic disk, is usually inferred from the radial expansion velocity of gas in the first ring. Our numerical hydrodynamics modeling of ring galaxy formation however shows …

2003 Astronomy and Astrophysics
eHST 14
pnCCDs on XMM-Newton—42 months in orbit
DOI: 10.1016/S0168-9002(03)01917-X Bibcode: 2003NIMPA.512..386S

Haberl, Frank; Freyberg, Michael; Dennerl, Konrad +11 more

XMM-Newton—a cornerstone mission of the European Space Agency's Horizon 2000 programme—was launched on December 10, 1999 into orbit. Since March 2000 more than 2000 scientific observations were made. An example will be shown. The X-ray pnCCD camera on EPIC is operating since then without severe problems. We will report about the system performance…

2003 Nuclear Instruments and Methods in Physics Research A
XMM-Newton 14
An analysis of the emission line spectra of AG Pegasi between phases 7.34 and 9.44
DOI: 10.1046/j.1365-8711.2003.06153.x Bibcode: 2003MNRAS.339..125C

Contini, Marcella

The UV and optical spectra from the HST Faint Object Spectrograph and from the Fast Spectrograph for the Tillinghast Telescope (FAST) spectrograph at the Whipple Observatory reported by Kenyon, Proga & Keyes at different phases are analysed, leading to new results about the configuration of AG Pegasi. The FAST spectra contain both Hα and Hβ li…

2003 Monthly Notices of the Royal Astronomical Society
eHST 14
870 Micron Observations of Nearby 3CRR Radio Galaxies
DOI: 10.1086/379562 Bibcode: 2003AJ....126.2677Q

Quillen, A. C.; Yukita, Mihoko; Almog, Jessica

We present submillimeter continuum observations at 870 µm of the cores of low-redshift 3CRR radio galaxies, observed at the Heinrich Hertz Submillimeter Telescope. The cores are nearly flat-spectrum between the radio and submillimeter, which implies that the submillimeter continuum is likely to be synchrotron emission and not thermal emissio…

2003 The Astronomical Journal
ISO eHST 14
Improved Hipparcos Parallaxes of Coma Berenices and NGC 6231
DOI: 10.1086/378483 Bibcode: 2003AJ....126.2408M

Makarov, Valeri V.

A method to reprocess the Hipparcos Intermediate Astrometry Data that reduces the propagation of the along-scan spacecraft attitude errors was developed and successfully used to obtain a more consistent parallax of the Pleiades (Makarov, published in 2002). The same technique is used now to correct the Hipparcos parallaxes of the Coma Berenices an…

2003 The Astronomical Journal
Hipparcos 14