Aims.We look for galactic neutral hydrogen (Hi) supershells likely to be associated with massive star groupings.Methods.A neutral hydrogen (Hi) line survey carried out at the Instituto Argentino de Radioastronomía (IAR) and the Southern Galactic Plane Survey (SGPS) were the main databases used in this investigation.Results.A new Hi supershell (GS263-02+45) was found in the outer part of the Galaxy. This structure is located at a distance of 5.3 1 kpc from the Sun and has a linear diameter of about 665 40 pc. The expansion velocity of the supershell is ~14 km s. The total amount of atomic gas related to GS263-02+45 is ~2 10 . Based on the analysis of the SGPS Hi data it is concluded that the OB-association Bochum 7 is likely to be interactin...
We present new high-resolution neutral hydrogen (H I) images of the Galactic supershell GSH 242-03+3...
We present new high resolution neutral hydrogen (H I) images of the Galactic supershell GSH 242-03+3...
Context. HI shells and supershells, found in discs of many galaxies including our own, are formed by...
Aims.We look for galactic neutral hydrogen (Hi) supershells likely to be associated with massive sta...
Aims: We look for galactic neutral hydrogen (Hi) supershells likely to be associated with massive st...
Neutral hydrogen (HI) supershells are usually identified, in a given velocity range, as a brightness...
We report on the discovery of a new Galactic supershell, GSH 006−15+7, from the Galactic All Sky Sur...
Aims. We carry out a multiwavelength study to characterize the H I supershell designated GS118+01-44...
Taking a clue from the pair of HI supershells found in the Scd galaxy NGC 3556 (M 108), we propose a...
Aims. The main goal of this work is to a have a new neutral hydrogen (H i) supershell candidate cata...
Context. The Milky Way, when viewed in the neutral hydrogen line emission, presents large structures...
Con. The Milky Way, when viewed in the neutral hydrogen line emission, presents large structures cal...
Context. Massive stars deeply modify their surrounding interstellar medium (ISM) via their high thro...
Context. Massive stars have a profound effect on the surrounding interstellar medium. They ionize an...
A New catalogue of H I supershell candidates (GSc) was developed in the outer part of the Galaxy. T...
We present new high-resolution neutral hydrogen (H I) images of the Galactic supershell GSH 242-03+3...
We present new high resolution neutral hydrogen (H I) images of the Galactic supershell GSH 242-03+3...
Context. HI shells and supershells, found in discs of many galaxies including our own, are formed by...
Aims.We look for galactic neutral hydrogen (Hi) supershells likely to be associated with massive sta...
Aims: We look for galactic neutral hydrogen (Hi) supershells likely to be associated with massive st...
Neutral hydrogen (HI) supershells are usually identified, in a given velocity range, as a brightness...
We report on the discovery of a new Galactic supershell, GSH 006−15+7, from the Galactic All Sky Sur...
Aims. We carry out a multiwavelength study to characterize the H I supershell designated GS118+01-44...
Taking a clue from the pair of HI supershells found in the Scd galaxy NGC 3556 (M 108), we propose a...
Aims. The main goal of this work is to a have a new neutral hydrogen (H i) supershell candidate cata...
Context. The Milky Way, when viewed in the neutral hydrogen line emission, presents large structures...
Con. The Milky Way, when viewed in the neutral hydrogen line emission, presents large structures cal...
Context. Massive stars deeply modify their surrounding interstellar medium (ISM) via their high thro...
Context. Massive stars have a profound effect on the surrounding interstellar medium. They ionize an...
A New catalogue of H I supershell candidates (GSc) was developed in the outer part of the Galaxy. T...
We present new high-resolution neutral hydrogen (H I) images of the Galactic supershell GSH 242-03+3...
We present new high resolution neutral hydrogen (H I) images of the Galactic supershell GSH 242-03+3...
Context. HI shells and supershells, found in discs of many galaxies including our own, are formed by...