The main objectives of the workshop were to review current observational evidence for spiral arms in our Galaxy and confront them with models of spiral structure in order to arrive at a consistent picture. Of primary importance was to understand just what additional information is required to resolve outstanding issues related to the spiral structure in the Milky Way, especially as new survey instruments (e.g., ALMA, VISTA and VST) are coming online and major space missions like GAIA will be launched in the near future
It was in 1864 that the first clues as to the nature of the space between stars were first identifie...
Context. The spiral structure of our Milky Way Galaxy is not yet known. HII regions and giant molecu...
We describe a system that builds quantitative structural descriptions of spiral galaxies. This enabl...
[Context] The physical processes driving the formation of Galactic spiral arms are still under debat...
Context. The astrometric satellite Gaia is expected to significantly increase our knowledge as to th...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
Between the early 40s, when Baade showed the first evidence for the existence of two distinct stella...
Abstract. Studying star formation in spiral arms tells us not only about the evolution of star forma...
Our home galaxy, the Milky Way, has been a focus of astrophysical research since before we knew ther...
European Space Agency (ESA)'s Gaia mission is providing the position, parallax and proper motions fo...
I will present the results of our investigation of the Gaia Phase Spiral using Gaia Data Release 3. ...
The census of stellar structures and star clusters in the Milky Way has been vastly improved in the ...
Context. Recent high-resolution observations have shown that stellar winds harbour complexities that...
We combine optical and radio observations to trace the spiral structure in the Third Quadrant of th...
International audienceThis is the second ESO workshop devoted to the topic of 3D spectroscopy of gal...
It was in 1864 that the first clues as to the nature of the space between stars were first identifie...
Context. The spiral structure of our Milky Way Galaxy is not yet known. HII regions and giant molecu...
We describe a system that builds quantitative structural descriptions of spiral galaxies. This enabl...
[Context] The physical processes driving the formation of Galactic spiral arms are still under debat...
Context. The astrometric satellite Gaia is expected to significantly increase our knowledge as to th...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
Between the early 40s, when Baade showed the first evidence for the existence of two distinct stella...
Abstract. Studying star formation in spiral arms tells us not only about the evolution of star forma...
Our home galaxy, the Milky Way, has been a focus of astrophysical research since before we knew ther...
European Space Agency (ESA)'s Gaia mission is providing the position, parallax and proper motions fo...
I will present the results of our investigation of the Gaia Phase Spiral using Gaia Data Release 3. ...
The census of stellar structures and star clusters in the Milky Way has been vastly improved in the ...
Context. Recent high-resolution observations have shown that stellar winds harbour complexities that...
We combine optical and radio observations to trace the spiral structure in the Third Quadrant of th...
International audienceThis is the second ESO workshop devoted to the topic of 3D spectroscopy of gal...
It was in 1864 that the first clues as to the nature of the space between stars were first identifie...
Context. The spiral structure of our Milky Way Galaxy is not yet known. HII regions and giant molecu...
We describe a system that builds quantitative structural descriptions of spiral galaxies. This enabl...