Photometry of a galactic field at l = 232°. b = -6°: The old open cluster Auner 1, The Norma-Cygnus spiral arm, and the signature of the warped galactic thick disk
We perform a detailed photometric study of the stellar populations in a Galactic field at l = 232°, b = -6° in the Canis Major (CMa) constellation. We present the first U, B, V, I photometry of the old open cluster Auner 1 and determine it to be ≈3.25 Gyr old and to lie 8.9 kpc from the Sun. In the...
Guardado en:
| Autores principales: | , , , , |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2007
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83126 |
| Aporte de: |
| id |
I19-R120-10915-83126 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Ciencias Astronómicas Galaxy: general Hertzsprung-Russell diagram Open clusters and associations: general Open clusters and associations: individual (Auner 1) |
| spellingShingle |
Ciencias Astronómicas Galaxy: general Hertzsprung-Russell diagram Open clusters and associations: general Open clusters and associations: individual (Auner 1) Carraro, Giovanni Moitinho, André Zoccali, Manuela Vázquez, Rubén Ángel Baume, Gustavo Photometry of a galactic field at l = 232°. b = -6°: The old open cluster Auner 1, The Norma-Cygnus spiral arm, and the signature of the warped galactic thick disk |
| topic_facet |
Ciencias Astronómicas Galaxy: general Hertzsprung-Russell diagram Open clusters and associations: general Open clusters and associations: individual (Auner 1) |
| description |
We perform a detailed photometric study of the stellar populations in a Galactic field at l = 232°, b = -6° in the Canis Major (CMa) constellation. We present the first U, B, V, I photometry of the old open cluster Auner 1 and determine it to be ≈3.25 Gyr old and to lie 8.9 kpc from the Sun. In the background of the cluster, at more than 9 kpc, we detect a young population most likely associated with the Norma-Cygnus spiral arm. Furthermore, we detect the signature of an older population and identify its turnoff and red giant branch. This population is found to have a mean age of 7 Gyr and a mean metallicity of Z = 0.006. We reconstruct the geometry of the stellar distribution and argue that this older population, often associated with the CMa "galaxy," in fact belongs to the warped old thin- and thick-disk components along this line of sight. |
| format |
Articulo Articulo |
| author |
Carraro, Giovanni Moitinho, André Zoccali, Manuela Vázquez, Rubén Ángel Baume, Gustavo |
| author_facet |
Carraro, Giovanni Moitinho, André Zoccali, Manuela Vázquez, Rubén Ángel Baume, Gustavo |
| author_sort |
Carraro, Giovanni |
| title |
Photometry of a galactic field at l = 232°. b = -6°: The old open cluster Auner 1, The Norma-Cygnus spiral arm, and the signature of the warped galactic thick disk |
| title_short |
Photometry of a galactic field at l = 232°. b = -6°: The old open cluster Auner 1, The Norma-Cygnus spiral arm, and the signature of the warped galactic thick disk |
| title_full |
Photometry of a galactic field at l = 232°. b = -6°: The old open cluster Auner 1, The Norma-Cygnus spiral arm, and the signature of the warped galactic thick disk |
| title_fullStr |
Photometry of a galactic field at l = 232°. b = -6°: The old open cluster Auner 1, The Norma-Cygnus spiral arm, and the signature of the warped galactic thick disk |
| title_full_unstemmed |
Photometry of a galactic field at l = 232°. b = -6°: The old open cluster Auner 1, The Norma-Cygnus spiral arm, and the signature of the warped galactic thick disk |
| title_sort |
photometry of a galactic field at l = 232°. b = -6°: the old open cluster auner 1, the norma-cygnus spiral arm, and the signature of the warped galactic thick disk |
| publishDate |
2007 |
| url |
http://sedici.unlp.edu.ar/handle/10915/83126 |
| work_keys_str_mv |
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Repositorios |
| _version_ |
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