Add to ORKGThis title from the Steward Observatory Preprints collection is made available by the Steward Observatory Parker Library and the University Libraries, The University of Arizona. If you have questions about titles in this collection, please contact Parker Library librarian Betty Fridena, bfridena@as.arizona.edu
Spiral arms dominate the appearance of most disk galaxies, like our own Milky Way, and have a signif...
We present a map of the spiral structure of the Galaxy, as traced by molecular carbon monosulphide (...
Original paper can be found at http://www.astrosociety.org/pubs/cs/222-252.html--Copyright Astronomi...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
SIGLEAvailable from British Library Document Supply Centre-DSC:DXN016862 / BLDSC - British Library D...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
The onset of spiral structure in galaxies appears to occur between redshifts 1.4 and 1.8 when disks ...
We combine optical and radio observations to trace the spiral structure in the Third Quadrant of th...
The main objectives of the workshop were to review current observational evidence for spiral arms in...
How does it happen that billions of stars can cooperate to produce the beautiful spirals that charac...
Context. The spiral structure of our Milky Way Galaxy is not yet known. HII regions and giant molecu...
Thesis examined at the University of Nottingham in April 2018, accepted in May 2018
It was in 1864 that the first clues as to the nature of the space between stars were first identifie...
Spiral arms dominate the appearance of most disk galaxies, like our own Milky Way, and have a signif...
We present a map of the spiral structure of the Galaxy, as traced by molecular carbon monosulphide (...
Original paper can be found at http://www.astrosociety.org/pubs/cs/222-252.html--Copyright Astronomi...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
SIGLEAvailable from British Library Document Supply Centre-DSC:DXN016862 / BLDSC - British Library D...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
This title from the Steward Observatory Preprints collection is made available by the Steward Observ...
The onset of spiral structure in galaxies appears to occur between redshifts 1.4 and 1.8 when disks ...
We combine optical and radio observations to trace the spiral structure in the Third Quadrant of th...
The main objectives of the workshop were to review current observational evidence for spiral arms in...
How does it happen that billions of stars can cooperate to produce the beautiful spirals that charac...
Context. The spiral structure of our Milky Way Galaxy is not yet known. HII regions and giant molecu...
Thesis examined at the University of Nottingham in April 2018, accepted in May 2018
It was in 1864 that the first clues as to the nature of the space between stars were first identifie...
Spiral arms dominate the appearance of most disk galaxies, like our own Milky Way, and have a signif...
We present a map of the spiral structure of the Galaxy, as traced by molecular carbon monosulphide (...
Original paper can be found at http://www.astrosociety.org/pubs/cs/222-252.html--Copyright Astronomi...
