Search Publications

On the Lyalpha emission from gamma-ray burst host galaxies: Evidence for low metallicities
DOI: 10.1051/0004-6361:20030931 Bibcode: 2003A&A...406L..63F

Fruchter, A. S.; Wijers, R. A. M. J.; Pedersen, H. +11 more

We report on the results of a search for Lyalpha emission from the host galaxy of the z=2.140 GRB 011211 and other galaxies in its surrounding field. We detect Lyalpha emission from the host as well as from six other galaxies in the field. The restframe equivalent width of the Lyalpha line from the GRB 011211 host is about 21 Å. This is the fifth …

2003 Astronomy and Astrophysics
eHST 154
Spectroscopic Binaries, Velocity Jitter, and Rotation in Field Metal-poor Red Giant and Red Horizontal-Branch Stars
DOI: 10.1086/345386 Bibcode: 2003AJ....125..293C

Latham, David W.; Stefanik, Robert P.; Morse, Jon A. +2 more

We summarize 2007 radial velocity measurements of 91 metal-poor field red giants. Excluding binary systems with orbital solutions, our coverage averages 13.7 yr per star, with a maximum of 18.0 yr. We report four significant findings. (1) Sixteen stars are found to be spectroscopic binaries, and we present orbital solutions for 14 of them. The spe…

2003 The Astronomical Journal
Hipparcos 154
Changes in Solar Dynamics from 1995 to 2002
DOI: 10.1086/346020 Bibcode: 2003ApJ...585..553B

Basu, Sarbani; Antia, H. M.

Data obtained by the GONG and MDI instruments over the last 7 years are used to study how solar dynamics-both rotation and other large scale flows-has changed with time. In addition to the well-known phenomenon of bands of faster and slower rotation moving toward the equator and pole, we find that the zonal flow pattern rises upward with time. Lik…

2003 The Astrophysical Journal
SOHO 153
The magnetic field of an isolated neutron star from X-ray cyclotron absorption lines
DOI: 10.1038/nature01703 Bibcode: 2003Natur.423..725B

Caraveo, P. A.; Bignami, G. F.; Mereghetti, S. +1 more

Isolated neutron stars are highly magnetized, fast-rotating objects that form as an end point of stellar evolution. They are directly observable in X-ray emission, because of their high surface temperatures. Features in their X-ray spectra could in principle reveal the presence of atmospheres, or be used to estimate the strength of their magnetic …

2003 Nature
XMM-Newton 151
Slow-mode standing waves observed by SUMER in hot coronal loops
DOI: 10.1051/0004-6361:20030448 Bibcode: 2003A&A...402L..17W

Solanki, S. K.; Marsch, E.; Curdt, W. +2 more

We report the first detection of postflare loop oscillations seen in both Doppler shift and intensity. The observations were recorded in an Fe Xix line by the SUMER spectrometer on SOHO in the corona about 70 min after an M-class flare on the solar limb. The oscillation has a period of about 17 min in both the Doppler velocity and the intensity, b…

2003 Astronomy and Astrophysics
SOHO 151
Dynamics of solar coronal loops. I. Condensation in cool loops and its effect on transition region lines
DOI: 10.1051/0004-6361:20031328 Bibcode: 2003A&A...411..605M

Peter, H.; Hansteen, V. H.; Müller, D. A. N.

We report numerical calculations of the condensation of plasma in short coronal loops, which have several interesting physical consequences. Firstly, we propose a connection between small, cool loops (T < 106 K), which constitute one of the basic components of the solar transition region, and prominences, in the sense that the same p…

2003 Astronomy and Astrophysics
SOHO 151
The low-level radial velocity variability in Barnard's star (= GJ 699). Secular acceleration, indications for convective redshift, and planet mass limits
DOI: 10.1051/0004-6361:20030396 Bibcode: 2003A&A...403.1077K

Kürster, M.; Hatzes, A. P.; Cochran, W. D. +6 more

We report results from 2 1/2 yr of high precision radial velocity (RV) monitoring of Barnard's star. The high RV measurement precision of the VLT-UT2+UVES of 2.65 m s-1 made the following findings possible. (1) The first detection of the change in the RV of a star caused by its space motion (RV secular acceleration). (2) An anti-correla…

2003 Astronomy and Astrophysics
Hipparcos 151
A pulsational approach to near-infrared and visual magnitudes of RR Lyr stars
DOI: 10.1046/j.1365-8711.2003.06878.x Bibcode: 2003MNRAS.344.1097B

Degl'Innocenti, S.; Marconi, M.; Bono, G. +3 more

In this paper, we present an improved theoretical scenario concerning near-infrared and visual magnitudes of RR Lyr variables, as based on up-to-date pulsating models. New relations connecting V and K absolute magnitudes with periods, mass, luminosity and metal content are discussed separately for fundamental and first-overtone pulsators. We also …

2003 Monthly Notices of the Royal Astronomical Society
eHST 151
Infrared Emission of Normal Galaxies from 2.5 to 12 Micron: Infrared Space Observatory Spectra, Near-Infrared Continuum, and Mid-Infrared Emission Features
DOI: 10.1086/374043 Bibcode: 2003ApJ...588..199L

Beichman, Charles A.; Dale, Daniel A.; Dinerstein, Harriet L. +6 more

We present ISOPHOT spectra of the regions 2.5-4.9 µm and 5.8-11.6 µm for a sample of 45 disk galaxies from the US Infrared Space Observatory Key Project on Normal Galaxies. The galaxies were selected to span the range in global properties of normal, star-forming disk galaxies in the local universe. The spectra can be decomposed into th…

2003 The Astrophysical Journal
ISO 150
Local galaxy flows within 5 Mpc
DOI: 10.1051/0004-6361:20021566 Bibcode: 2003A&A...398..479K

Sarajedini, A.; Dolphin, A. E.; Grebel, E. K. +8 more

We present Hubble Space Telescope/WFPC2 images of sixteen dwarf galaxies as part of our snapshot survey of nearby galaxy candidates. We derive their distances from the luminosity of the tip of the red giant branch stars with a typical accuracy of ~ 12%. The resulting distances are 4.26 Mpc (KKH 5), 4.74 Mpc (KK 16), 4.72 Mpc (KK 17), 4.66 Mpc (ESO…

2003 Astronomy and Astrophysics
eHST 150