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An XMM-Newton observation of the multiple system HD 167971 (O5-8V + O5-8V + (O8I)) and the young open cluster NGC 6604
DOI: 10.1051/0004-6361:20052810 Bibcode: 2005A&A...437.1029D

Blomme, R.; Rauw, G.; De Becker, M. +3 more

We discuss the results of two XMM-Newton observations of the open cluster NGC 6604 obtained in April and September 2002. We concentrate mainly on the multiple system HD 167971 (O5-8V + O5-8V + (O8I)). The soft part of the EPIC spectrum of this system is thermal with typical temperatures of about 2 × 106 to 9 × 106 K. The natu…

2005 Astronomy and Astrophysics
XMM-Newton 23
Statistics of high-altitude and high-latitude O+ ion outflows observed by Cluster/CIS
DOI: 10.5194/angeo-23-1909-2005 Bibcode: 2005AnGeo..23.1909A

Lundin, R.; Yamauchi, M.; Nilsson, H. +8 more

The persistent outflows of O+ ions observed by the Cluster CIS/CODIF instrument were studied statistically in the high-altitude (from 3 up to 11 RE) and high-latitude (from 70 to ~90 deg invariant latitude, ILAT) polar region. The principal results are: (1) Outflowing O+ ions with more than 1keV are observed above …

2005 Annales Geophysicae
Cluster 23
The very low-mass population of the Corona Australis and Chamaeleon II star forming regions
DOI: 10.1051/0004-6361:20053465 Bibcode: 2005A&A...444..175L

Eislöffel, J.; López Martí, B.; Mundt, R.

We present the results of a deep optical survey in the Corona Australis and Chamaeleon II star forming regions. Our optical photometry is combined with available near- and mid-infrared photometry to identify very low-mass candidate members in these dark clouds. In our Chamaeleon II field, only one object exhibits clear Hα emission, but the discrep…

2005 Astronomy and Astrophysics
ISO 23
Far Ultraviolet Spectroscopic Explorer Observations of the Symbiotic Star AG Draconis
DOI: 10.1086/426045 Bibcode: 2005ApJ...618..891Y

Young, P. R.; Dupree, A. K.; Espey, B. R. +2 more

Spectra of the bright symbiotic star AG Draconis (BD +67°922) in the wavelength range 905-1187 Å obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE) are presented. The spectra show a number of narrow, nebular emission lines, together with a uniform continuum from the hot component of the system, and numerous interstellar absorption lin…

2005 The Astrophysical Journal
IUE 23
A possible bright blue supernova in the afterglow of GRB 020305
DOI: 10.1051/0004-6361:20052783 Bibcode: 2005A&A...437..411G

Nugent, P.; Fynbo, J. P. U.; Gorosabel, J. +8 more

We report on ground-based and HST(+STIS) imaging of the afterglow and host galaxy of the Gamma-Ray Burst (GRB) of March 5, 2002. The GRB occurred in a R=25.17 ± 0.14 galaxy, which apparently is part of an interacting system. The lightcurve of the optical afterglow shows a rebrightening, or at least a plateau, 12 16 days after the gamma-ray event. …

2005 Astronomy and Astrophysics
eHST 23
RR Lyrae stars: kinematics, orbits and z-distribution
DOI: 10.1051/0004-6361:20053231 Bibcode: 2005A&A...442..229M

de Boer, K. S.; Maintz, G.

RR Lyrae stars in the Milky Way are good tracers to study the kinematic behaviour and spatial distribution of older stellar populations. A recently established well documented sample of 217 RR Lyr stars with V<12.5 mag, for which accurate distances and radial velocities as well as proper motions from the Hipparcos and Tycho-2 catalogues are ava…

2005 Astronomy and Astrophysics
Hipparcos 23
An X-Ray View of Weak-Line Radio Galaxies/LINERs
DOI: 10.1086/426708 Bibcode: 2005ApJ...621..167R

Gliozzi, Mario; Sambruna, Rita M.; Rinn, Alexander S.

We present X-ray observations of nine weak-line radio galaxies (WLRGs), optically classified as confirmed or possible LINERs. The data were taken from the Chandra, XMM-Newton, and BeppoSAX archives. The Chandra images typically show complex X-ray morphologies, with hard (2-10 keV) point sources embedded in diffuse soft (0.3-2.0 keV) emission in al…

2005 The Astrophysical Journal
XMM-Newton 23
New runaway OB stars with HIPPARCOS
DOI: 10.1051/0004-6361:200400134 Bibcode: 2005A&A...431L...1M

Mdzinarishvili, T. G.; Chargeishvili, K. B.

A Monte Carlo method for detection of runaway OB stars from observational data is proposed. 61 runaway OB star candidates have been detected by an analysis of Hipparcos proper motions. The peculiar tangential and total transverse velocities have been determined for these stars. A list of the detected runaway star candidates is presented. The evide…

2005 Astronomy and Astrophysics
Hipparcos 23
Kinetic Helicity Density in Solar Subsurface Layers and Flare Activity of Active Regions
DOI: 10.1086/432031 Bibcode: 2005ApJ...630.1184K

Howe, R.; Komm, R.; Hill, F. +2 more

We search for a relation between subsurface flows below active regions and flare events occurring in those regions. For this purpose, we use a ring-diagram analysis to determine the subsurface flows from high-resolution Global Oscillation Network Group (GONG) and Michelson Doppler Imager (MDI) data and derive the kinetic helicity as a measure of t…

2005 The Astrophysical Journal
SOHO 23
The influence of gravitational lensing on the spectra of lensed quasi-stellar objects
DOI: 10.1111/j.1365-2966.2004.08619.x Bibcode: 2005MNRAS.357..135P

Popović, L. Č.; Chartas, G.

We consider the influence of (milli/micro)lensing on the spectra of lensed quasi-stellar objects (QSOs). We propose a method for the observational detection of microlensing in the spectra of lensed QSOs and apply it to the spectra of three lensed QSOs (PG 1115+080, Q1413+117 and Q0957+561) observed with the Hubble Space Telescope. We find that the…

2005 Monthly Notices of the Royal Astronomical Society
eHST 23