Aims. We carry out a multiwavelength study to characterize the H i supershell designated GS 118+01−44, and to analyse its possible origin. Methods. A multiwavelength study has been carried out to study the supershell and its environs. We performed an analysis of the H i, CO, radio continuum, and infrared emission distributions. Results. The Canadian Galactic Plane Survey (CGPS) H i data reveals that GS 118+01−44 is centred at (l,b) = (117°̣7, 1°̣4) with a systemic velocity of −44.3 km s-1. According to Galactic rotation models this structure is located at 3.0 ± 0.6 kpc from the Sun. There are several H ii regions and three supernova remnants (SNRs) catalogued in the region. On the other hand, the analysis of the temperature spectral ind...
Original article can be found at: http://www.journals.uchicago.edu/ApJ/--Copyright American Astronom...
Context. The identification of counterparts of dark gamma-ray sources adds greatly to our understand...
Context. The Milky Way, when viewed in the neutral hydrogen line emission, presents large structures...
Aims. We carry out a multiwavelength study to characterize the H I supershell designated GS118+01-44...
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...
Aims: We look for galactic neutral hydrogen (Hi) supershells likely to be associated with massive st...
Context. Massive stars have a profound effect on the surrounding interstellar medium. They ionize an...
Context. Massive stars have a profound effect on the surrounding interstellar medium. They ionize an...
GSH 91.5 + 2 − 114 is a large H i shell located in the outer Galaxy at a kinematic distance of about...
Aims.We look for galactic neutral hydrogen (Hi) supershells likely to be associated with massive sta...
We present a multi-wavelength investigation of the H ii region G347.600+00.211, located at a distanc...
We report on the discovery of a new Galactic supershell, GSH 006−15+7, from the Galactic All Sky Sur...
A New catalogue of H I supershell candidates (GSc) was developed in the outer part of the Galaxy. T...
Aims. The main goal of this work is to a have a new neutral hydrogen (H i) supershell candidate cata...
Original article can be found at: http://www.journals.uchicago.edu/ApJ/--Copyright American Astronom...
Context. The identification of counterparts of dark gamma-ray sources adds greatly to our understand...
Context. The Milky Way, when viewed in the neutral hydrogen line emission, presents large structures...
Aims. We carry out a multiwavelength study to characterize the H I supershell designated GS118+01-44...
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...
Aims: We look for galactic neutral hydrogen (Hi) supershells likely to be associated with massive st...
Context. Massive stars have a profound effect on the surrounding interstellar medium. They ionize an...
Context. Massive stars have a profound effect on the surrounding interstellar medium. They ionize an...
GSH 91.5 + 2 − 114 is a large H i shell located in the outer Galaxy at a kinematic distance of about...
Aims.We look for galactic neutral hydrogen (Hi) supershells likely to be associated with massive sta...
We present a multi-wavelength investigation of the H ii region G347.600+00.211, located at a distanc...
We report on the discovery of a new Galactic supershell, GSH 006−15+7, from the Galactic All Sky Sur...
A New catalogue of H I supershell candidates (GSc) was developed in the outer part of the Galaxy. T...
Aims. The main goal of this work is to a have a new neutral hydrogen (H i) supershell candidate cata...
Original article can be found at: http://www.journals.uchicago.edu/ApJ/--Copyright American Astronom...
Context. The identification of counterparts of dark gamma-ray sources adds greatly to our understand...
Context. The Milky Way, when viewed in the neutral hydrogen line emission, presents large structures...