The Spectrum of RS Ophiuchi during the 1958 maximum
- Autores
- Gratton, Livio; Landi Dessy, Jorge
- Año de publicación
- 1961
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The recurrent Nova RS Oph brightened to the 6th magnitude between July 13 and 14 1958. This is the third observed outburst of this variable; the other two occurred in 1898 and 1933 (Cecchini and Gratton 1941). The news of the outburst reached Córdoba the 15th of July and a dozen of spectroscopic plates were obtained by the Authors from July 15.9 to July 25.0 at Bosque Alegre with the standard equipment ( 60" Reflector, grating spectrograph with a dispersion of 42 A/mm). Buring the time of the observations, apparently, the star reached a maximum (around July 18) and began to fade slowly. (Párrafo extraído a modo de resumen)
Asociación Argentina de Astronomía - Materia
-
Astronomía
Galaxias - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/73460
Ver los metadatos del registro completo
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The Spectrum of RS Ophiuchi during the 1958 maximumGratton, LivioLandi Dessy, JorgeAstronomíaGalaxiasThe recurrent Nova RS Oph brightened to the 6th magnitude between July 13 and 14 1958. This is the third observed outburst of this variable; the other two occurred in 1898 and 1933 (Cecchini and Gratton 1941). The news of the outburst reached Córdoba the 15th of July and a dozen of spectroscopic plates were obtained by the Authors from July 15.9 to July 25.0 at Bosque Alegre with the standard equipment ( 60" Reflector, grating spectrograph with a dispersion of 42 A/mm). Buring the time of the observations, apparently, the star reached a maximum (around July 18) and began to fade slowly. <i>(Párrafo extraído a modo de resumen)</i>Asociación Argentina de Astronomía1961info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/73460enginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:12:26Zoai:sedici.unlp.edu.ar:10915/73460Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:12:26.907SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
The Spectrum of RS Ophiuchi during the 1958 maximum |
| title |
The Spectrum of RS Ophiuchi during the 1958 maximum |
| spellingShingle |
The Spectrum of RS Ophiuchi during the 1958 maximum Gratton, Livio Astronomía Galaxias |
| title_short |
The Spectrum of RS Ophiuchi during the 1958 maximum |
| title_full |
The Spectrum of RS Ophiuchi during the 1958 maximum |
| title_fullStr |
The Spectrum of RS Ophiuchi during the 1958 maximum |
| title_full_unstemmed |
The Spectrum of RS Ophiuchi during the 1958 maximum |
| title_sort |
The Spectrum of RS Ophiuchi during the 1958 maximum |
| dc.creator.none.fl_str_mv |
Gratton, Livio Landi Dessy, Jorge |
| author |
Gratton, Livio |
| author_facet |
Gratton, Livio Landi Dessy, Jorge |
| author_role |
author |
| author2 |
Landi Dessy, Jorge |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Astronomía Galaxias |
| topic |
Astronomía Galaxias |
| dc.description.none.fl_txt_mv |
The recurrent Nova RS Oph brightened to the 6th magnitude between July 13 and 14 1958. This is the third observed outburst of this variable; the other two occurred in 1898 and 1933 (Cecchini and Gratton 1941). The news of the outburst reached Córdoba the 15th of July and a dozen of spectroscopic plates were obtained by the Authors from July 15.9 to July 25.0 at Bosque Alegre with the standard equipment ( 60" Reflector, grating spectrograph with a dispersion of 42 A/mm). Buring the time of the observations, apparently, the star reached a maximum (around July 18) and began to fade slowly. <i>(Párrafo extraído a modo de resumen)</i> Asociación Argentina de Astronomía |
| description |
The recurrent Nova RS Oph brightened to the 6th magnitude between July 13 and 14 1958. This is the third observed outburst of this variable; the other two occurred in 1898 and 1933 (Cecchini and Gratton 1941). The news of the outburst reached Córdoba the 15th of July and a dozen of spectroscopic plates were obtained by the Authors from July 15.9 to July 25.0 at Bosque Alegre with the standard equipment ( 60" Reflector, grating spectrograph with a dispersion of 42 A/mm). Buring the time of the observations, apparently, the star reached a maximum (around July 18) and began to fade slowly. <i>(Párrafo extraído a modo de resumen)</i> |
| publishDate |
1961 |
| dc.date.none.fl_str_mv |
1961 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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http://sedici.unlp.edu.ar/handle/10915/73460 |
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eng |
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eng |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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