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XMM-Newton observations of two black hole X-ray transients in quiescence
DOI: 10.1051/0004-6361:20021746 Bibcode: 2003A&A...399..631H

Motch, C.; McClintock, J. E.; Barret, D. +5 more

We report on XMM-Newton observations of GRO J1655-40 and GRS 1009-45, which are two black hole X-ray transients currently in their quiescent phase. GRO J1655-40 was detected with a 0.5-10 keV luminosity of 5.9 x 1031 erg s-1 with 20% accuracy, taking into account both statistical errors and uncertainty on the distance. This l…

2003 Astronomy and Astrophysics
XMM-Newton 52
Damped Lyα Gas Metallicities at Redshifts z=0.9-2.0 from Sloan Digital Sky Survey Spectra
DOI: 10.1086/378841 Bibcode: 2003ApJ...595L...5N

Turnshek, David A.; Rao, Sandhya M.; Vanden Berk, Daniel +1 more

Using Sloan Digital Sky Survey early data release spectra, we have identified 370 Mg II absorption systems with Mg II λ2796 rest equivalent widths >=1 Å and redshifts z=0.9-2.2. From our previous and ongoing Hubble Space Telescope UV spectroscopic studies, we estimate that the mean neutral hydrogen column density of a system selected in this ma…

2003 The Astrophysical Journal
eHST 52
An Extended Burst Tail from SGR 1900+14 with a Thermal X-Ray Spectrum
DOI: 10.1086/368343 Bibcode: 2003ApJ...587..761L

Hurley, Kevin; Kouveliotou, Chryssa; Göǧüş, Ersin +6 more

The soft gamma repeater SGR 1900+14 entered a new phase of activity in 2001 April initiated by the intermediate flare recorded on April 18. Ten days following this flare, we discovered an abrupt increase in the source flux between consecutive Rossi X-Ray Timing Explorer (RXTE) orbits. This X-ray flux excess decayed over the next several minutes an…

2003 The Astrophysical Journal
Ulysses 52
Circumstellar features in hot DA white dwarfs
DOI: 10.1046/j.1365-8711.2003.06409.x Bibcode: 2003MNRAS.341..477B

Barstow, M. A.; Bruhweiler, F. C.; Holberg, J. B. +1 more

We present a phenomenological study of highly ionized, non-photospheric absorption features in high spectral resolution vacuum ultraviolet spectra of 23 hot DA white dwarfs. Prior to this study, four of the survey objects (Feige 24, REJ 0457-281, G191-B2B and REJ 1614-085) were known to possess these features. We find four new objects with multipl…

2003 Monthly Notices of the Royal Astronomical Society
IUE eHST 52
Proper Motions of Open Star Clusters and the Rotation Rate of the Galaxy
DOI: 10.1134/1.1538491 Bibcode: 2003ARep...47....6L

Beshenov, G. V.; Loktin, A. V.

The mean proper motions of 167 Galactic open clusters with radial-velocity measurements are computed from the data of the Tycho-2 catalog using kinematic and photometric cluster membership criteria. The resulting catalog is compared to the results of other studies. The new proper motions are used to infer the Galactic rotation rate at the solar ci…

2003 Astronomy Reports
Hipparcos 52
Quasi-periodic Pulsations in a Solar Microwave Burst
DOI: 10.1086/374315 Bibcode: 2003ApJ...588.1163G

Kundu, M. R.; White, S. M.; Grechnev, V. V.

Quasi-periodic pulsations in solar flares can provide important information on physical conditions in flaring regions. In this paper, we study a microwave burst that showed deep quasi-periodic pulsations. The most dramatic feature of this event has been discussed by Asai and coworkers. In the second of four bursts during the flare, strongly modula…

2003 The Astrophysical Journal
SOHO 52
A Hubble Space Telescope WFPC2 Investigation of the Nuclear Morphology in the Toomre Sequence of Merging Galaxies
DOI: 10.1086/379676 Bibcode: 2003AJ....126.2717L

Böker, Torsten; van der Marel, Roeland P.; Zabludoff, Ann I. +4 more

We report on the properties of nuclear regions in the Toomre sequence of merging galaxies, based on imaging data gathered with the Hubble Space Telescope WFPC2 camera. We have imaged the 11 systems in the proposed evolutionary merger sequence in the F555W and F814W broadband filters, and in Hα+[N II] narrowband filters. The broadband morphology of…

2003 The Astronomical Journal
eHST 51
The high frequency power spectrum of Markarian 766
DOI: 10.1046/j.1365-8711.2003.06415.x Bibcode: 2003MNRAS.341..496V

Vaughan, S.; Fabian, A. C.

An analysis is presented of the power spectrum of X-ray variability of the bright Seyfert 1 galaxy Mrk 766 as observed by XMM-Newton. Over the 0.2-10 keV energy range the power spectral density (PSD) is well-represented by a power-law with a slope of αlow~ 1 at low frequencies, breaking to a slope of αhi= 2.8+0.2

2003 Monthly Notices of the Royal Astronomical Society
XMM-Newton 51
Detection of strongly processed ice in the central starburst of NGC 4945
DOI: 10.1051/0004-6361:20030290 Bibcode: 2003A&A...402..499S

Lutz, D.; Pontoppidan, K. M.; Tielens, A. G. G. M. +4 more

The composition of ice grains provides an important tool for the study of the molecular environment of star forming regions. Using ISAAC at the VLT to obtain spectra around 4.65 mu m we have detected for the first time ``XCN'' and CO ice in an extragalactic environment: the nuclear region of the nearby dusty starburst/AGN galaxy NGC 4945. The prof…

2003 Astronomy and Astrophysics
eHST 51
Balmer Lines as Diagnostics of Physical Conditions in Active Galactic Nuclei Broad Emission Line Regions
DOI: 10.1086/376401 Bibcode: 2003ApJ...599..140P

Popović, L. Č.

Using a well-known method for laboratory plasma diagnostics, the Boltzmann plot, we discuss the physical properties in the broad-line regions (BLRs) of active galactic nuclei (AGNs). We apply the Boltzmann plot method to Balmer lines on a sample of 14 AGNs and find that it may indicate the existence of ``case B'' recombination or partial local the…

2003 The Astrophysical Journal
eHST 51