Discovery and statistics of Be stars
In 1960, the authors have started at the La Plata Observatory a survey of bright B stars (m ≤ 6.5, δ< 0°, HD Spectral type 09-B5) for the discovery of emission in Hα. A two prism spectrograph attached to the 80 cm La Plata telescope was used, with a camera giving a dispersion of 180 A/mm. The sli...
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| Formato: | Articulo |
| Lenguaje: | Inglés |
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1962
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/77002 |
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I19-R120-10915-770022024-05-23T18:57:22Z http://sedici.unlp.edu.ar/handle/10915/77002 Discovery and statistics of Be stars Jaschek, Carlos Jaschek, Mercedes Kucewicz, Boris 1962 2019-06-24T17:14:11Z en Ciencias Astronómicas B stars spectrograph In 1960, the authors have started at the La Plata Observatory a survey of bright B stars (m ≤ 6.5, δ< 0°, HD Spectral type 09-B5) for the discovery of emission in Hα. A two prism spectrograph attached to the 80 cm La Plata telescope was used, with a camera giving a dispersion of 180 A/mm. The slit was opened as much as possible in order to shorten the exposure times; as a consequence the region of good definition on the plates comprises only from 6000 to 6700 A. Asociación Argentina de Astronomía Articulo Articulo http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 37-41 |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Ciencias Astronómicas B stars spectrograph |
| spellingShingle |
Ciencias Astronómicas B stars spectrograph Jaschek, Carlos Jaschek, Mercedes Kucewicz, Boris Discovery and statistics of Be stars |
| topic_facet |
Ciencias Astronómicas B stars spectrograph |
| description |
In 1960, the authors have started at the La Plata Observatory a survey of bright B stars (m ≤ 6.5, δ< 0°, HD Spectral type 09-B5) for the discovery of emission in Hα. A two prism spectrograph attached to the 80 cm La Plata telescope was used, with a camera giving a dispersion of 180 A/mm. The slit was opened as much as possible in order to shorten the exposure times; as a consequence the region of good definition on the plates comprises only from 6000 to 6700 A. |
| format |
Articulo Articulo |
| author |
Jaschek, Carlos Jaschek, Mercedes Kucewicz, Boris |
| author_facet |
Jaschek, Carlos Jaschek, Mercedes Kucewicz, Boris |
| author_sort |
Jaschek, Carlos |
| title |
Discovery and statistics of Be stars |
| title_short |
Discovery and statistics of Be stars |
| title_full |
Discovery and statistics of Be stars |
| title_fullStr |
Discovery and statistics of Be stars |
| title_full_unstemmed |
Discovery and statistics of Be stars |
| title_sort |
discovery and statistics of be stars |
| publishDate |
1962 |
| url |
http://sedici.unlp.edu.ar/handle/10915/77002 |
| work_keys_str_mv |
AT jaschekcarlos discoveryandstatisticsofbestars AT jaschekmercedes discoveryandstatisticsofbestars AT kucewiczboris discoveryandstatisticsofbestars |
| _version_ |
1807220389143642112 |