To elucidate the nature of the interstellar medium in the vicinity of the Vela supernova remnants (SNR) an extensive study with the International Ultraviolet Explorer of interstellar absorption lines toward 35 stars in the vicinity of the Vela SNR was undertaken. Observations of interstellar absorption, in particular of CI, towards one of these stars, HD 72350 (type B4 III), is of particular interest
Conference: High energy gamma-ray astronomy: 6th International Meeting on High Energy Gamma-ray Astr...
Supernova remnants (SNRs), which are very energetic objects, are thought to have great influence on ...
Using the IRAM 30-m telescope, we observed the supernova remnant 3C391 (G31.9+0.0) and its surroundi...
Aims. Supernova remnant (SNR) RX J0852.0-4622 is one of the youngest and is most likely the closest ...
Highly ionized gas, in particular C IV and O VI, is produced in the interstellar medium in regions w...
We present an analysis of high-resolution far-UV archival spectra obtained with the Space Telescope ...
In a search for molecular gas associated with supernova remnants, the CO line has been observed in t...
Unusually strong high-excitation C I has been detected in eleven lines of sight through the Vela sup...
The interaction of the SNR 3C 400.2 with the interstellar medium is investigated on the basis of the...
We present the results of a new high-resolution study of the molecular gas associated with the supe...
The star HD72089 is located behind the Vela supernova remnant and shows a complex array of high and ...
xi, 112 leaves : ill. ; 28 cm.Includes abstract.Includes bibliographical references (leaves 97-102)....
The primary interest was to analyze the interstellar lines produced by gases along the line of sight...
XMM-Newton spatial/spectral resolution and high effective area allow to deepen our knowledge about t...
We study the geometry and dynamics of the Vela complex including the Vela supernova remnan...
Conference: High energy gamma-ray astronomy: 6th International Meeting on High Energy Gamma-ray Astr...
Supernova remnants (SNRs), which are very energetic objects, are thought to have great influence on ...
Using the IRAM 30-m telescope, we observed the supernova remnant 3C391 (G31.9+0.0) and its surroundi...
Aims. Supernova remnant (SNR) RX J0852.0-4622 is one of the youngest and is most likely the closest ...
Highly ionized gas, in particular C IV and O VI, is produced in the interstellar medium in regions w...
We present an analysis of high-resolution far-UV archival spectra obtained with the Space Telescope ...
In a search for molecular gas associated with supernova remnants, the CO line has been observed in t...
Unusually strong high-excitation C I has been detected in eleven lines of sight through the Vela sup...
The interaction of the SNR 3C 400.2 with the interstellar medium is investigated on the basis of the...
We present the results of a new high-resolution study of the molecular gas associated with the supe...
The star HD72089 is located behind the Vela supernova remnant and shows a complex array of high and ...
xi, 112 leaves : ill. ; 28 cm.Includes abstract.Includes bibliographical references (leaves 97-102)....
The primary interest was to analyze the interstellar lines produced by gases along the line of sight...
XMM-Newton spatial/spectral resolution and high effective area allow to deepen our knowledge about t...
We study the geometry and dynamics of the Vela complex including the Vela supernova remnan...
Conference: High energy gamma-ray astronomy: 6th International Meeting on High Energy Gamma-ray Astr...
Supernova remnants (SNRs), which are very energetic objects, are thought to have great influence on ...
Using the IRAM 30-m telescope, we observed the supernova remnant 3C391 (G31.9+0.0) and its surroundi...