Nova Puppis 1673
In this article, we want to address Nova Puppis 1673 from a comprehensive approach, analyzing its different facets and its impact on today's society. Nova Puppis 1673 is a topic that has generated great interest in recent years, due to its relevance in various areas, from politics to popular culture. Through a detailed analysis, we aim to offer a broad and deep vision of Nova Puppis 1673, addressing its history, its current implications and possible future prospects. This article seeks to be an informative and reflective tool for those who wish to better understand Nova Puppis 1673 and its implications in contemporary society.
 Location of Nova Puppis 1673 (circled in red) | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Puppis |
| Right ascension | 07h 59m 01.0s[1] |
| Declination | −43° 49′ 06″[1] |
| Apparent magnitude (V) | 3.0 – 20.0[2] |
| Characteristics | |
| Variable type | Nova?[2] |
| Other designations | |
| NSV 3846, Zi 816 | |
| Database references | |
| SIMBAD | data |
Nova Puppis 1673, also known as NSV 3846, is a probable nova in the constellation Puppis. It was discovered by French astronomer Jean Richer on January 12, 1673 (and again observed on January 21) during the last year of an expedition Richer made to Cayenne, French Guiana. Richer measured its position on the sky using a mural quadrant, resulting in the most precise position available for a seventeenth-century nova that might be rediscovered by modern observers. At the time of its discovery the nova had a visual magnitude of 3, making it easily visible to the naked eye.[3][4][5]
In 1987, German astronomer Hilmar Duerbeck published an ESO photographic survey image, marked with the position of a 20th magnitude candidate for a modern identification of Nova Puppis 1673.[3] However subsequent spectral observations of that potential remnant of the nova showed narrow Balmer absorption lines against a blue continuum, features which are not typically seen in quiescent novae. Hence, Duerbeck's proposed identification could not be confirmed.[5]
References
- ^ a b Downes, Ronald; Webbink, Ronald F.; Shara, Michael M. (April 1997). "A Catalog and Atlas of Cataclysmic Variables-Second Edition". Publications of the Astronomical Society of the Pacific. 109: 345–440. Bibcode:1997PASP..109..345D. doi:10.1086/133900. S2CID 120396435.
- ^ a b "NSV 3846". The International Variable Star Index. AAVSO. Retrieved 4 October 2022.
- ^ a b Duerbeck, Hilmar W. (March 1987). "A Reference Catalogue and Atlas of Galactic Novae". Space Science Reviews. 45 (1–2): 1–14. Bibcode:1987SSRv...45....1D. doi:10.1007/BF00187826. S2CID 115854775.
- ^ Olmsted, John W (1942). "The Scientific Expedition of Jean Richer to Cayenne (1672-1673)". Isis. 34 (2): 117–128. Bibcode:1942Isis...34..117O. doi:10.1086/347762. JSTOR 226212. S2CID 144341198.
- ^ a b Shara, Michael M.; Moffat, Anthony F. J.; Potter, Michael (August 1990). "Spectroscopic Authentication of Very Old Nova Candidates". Astronomical Journal. 100: 540. Bibcode:1990AJ....100..540S. doi:10.1086/115535.
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