Evidence of ongoing radial migration in NGC 6754: azimuthal variations of the gas properties
Understanding the nature of spiral structure in disk galaxies is one of the main, and still unsolved, questions in galactic astronomy. However, theoretical works are proposing new testable predictions whose detection is becoming feasible with recent development in instrumentation. In particular, str...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2016 October 20
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| In: |
The astrophysical journal. Part 2, Letters
Year: 2016, Volume: 830, Issue: 2 |
| ISSN: | 2041-8213 |
| DOI: | 10.3847/2041-8205/830/2/L40 |
| Online Access: | Verlag, Volltext: http://dx.doi.org/10.3847/2041-8205/830/2/L40
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| Author Notes: | L. Sánchez-Menguiano, S.F. Sánchez, D. Kawata, L. Chemin, I. Pérez, T. Ruiz-Lara, P. Sánchez-Blázquez, L. Galbany, J.P. Anderson, R.J.J. Grand, I. Minchev, and F.A. Gómez |
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Evidence of ongoing radial migration in NGC 6754: azimuthal variations of the gas properties
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