Context. The role of massive stars is central to an understanding of galactic ecology. It is important to establish the details of how massive stars provide radiative, chemical, and mechanical feedback in galaxies. Central to these issues is an understanding of the evolution of massive stars, and the critical role of mass loss via strongly structured winds and stellar binarity. Ultimately, and acting collectively, massive stellar clusters shape the structure and energetics of galaxies. Aims. We aim to conduct high-resolution, deep field mapping at 21 cm of the core of the massive Cygnus OB2 association and to characterise the properties of the massive stars and colliding winds at this waveband. Methods. We used seven stations of the e-MERLI...
We report on the analysis of the Chandra-ACIS data of O, B, and WR stars in the young association Cy...
© 2023, The Author(s). Published by the American Astronomical Society. This is an open access articl...
This is the final version of the article. Available from the American Astronomical Society via the D...
Context. The role of massive stars is central to an understanding of galactic ecology. It is importa...
Context. The role of massive stars is central to an understanding of galactic ecology. It is importa...
We present e-MERLIN 21 cm (L-band) observations of single luminous OB stars in the Cygnus OB2 associ...
Context. The Cygnus complex is one of the most powerful star forming regions at a close distance fro...
We present results of a high angular resolution survey of massive OB stars in the Cygnus OB2 associa...
We conducted a radial velocity survey of the Cyg OB2 association over a 6 yr (1999-2005) time interv...
We present a radio continuum survey at 1400 and 350 MHz of a region of 2degrees x 2degrees centered ...
We conducted a radial velocity survey of the Cygnus OB2 Association over a 6 year (1999 - 2005) time...
Context. Cyg OB2 is one of the most massive associations of O-type stars in our Galaxy. Despite the ...
Context. The compact association Cygnus OB2 is known to contain a large population of massive stars...
We present results of a high angular resolution survey of massive OB stars in the Cygnus OB2 associa...
We have compiled a significantly updated and comprehensive census of massive stars in the nearby Cyg...
We report on the analysis of the Chandra-ACIS data of O, B, and WR stars in the young association Cy...
© 2023, The Author(s). Published by the American Astronomical Society. This is an open access articl...
This is the final version of the article. Available from the American Astronomical Society via the D...
Context. The role of massive stars is central to an understanding of galactic ecology. It is importa...
Context. The role of massive stars is central to an understanding of galactic ecology. It is importa...
We present e-MERLIN 21 cm (L-band) observations of single luminous OB stars in the Cygnus OB2 associ...
Context. The Cygnus complex is one of the most powerful star forming regions at a close distance fro...
We present results of a high angular resolution survey of massive OB stars in the Cygnus OB2 associa...
We conducted a radial velocity survey of the Cyg OB2 association over a 6 yr (1999-2005) time interv...
We present a radio continuum survey at 1400 and 350 MHz of a region of 2degrees x 2degrees centered ...
We conducted a radial velocity survey of the Cygnus OB2 Association over a 6 year (1999 - 2005) time...
Context. Cyg OB2 is one of the most massive associations of O-type stars in our Galaxy. Despite the ...
Context. The compact association Cygnus OB2 is known to contain a large population of massive stars...
We present results of a high angular resolution survey of massive OB stars in the Cygnus OB2 associa...
We have compiled a significantly updated and comprehensive census of massive stars in the nearby Cyg...
We report on the analysis of the Chandra-ACIS data of O, B, and WR stars in the young association Cy...
© 2023, The Author(s). Published by the American Astronomical Society. This is an open access articl...
This is the final version of the article. Available from the American Astronomical Society via the D...