Suggested Stellar Transients - Revision history

Sushoff at 19:36, 19 February 2026

2026-02-19T19:36:21Z

← Older revision		Revision as of 19:36, 19 February 2026
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			{{PAGEAUTHORS}}
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	In the 1930s, Walter Baade and Fritz Zwicky developed the hypothesis of stars that end their lives in big explosions: supernovae. Only in the 1960s, in a series of three papers by Robert Krafft, the physical nature of novae was explained as surface eruptions on white dwarf stars in cataclysmic binary systems.		In the 1930s, Walter Baade and Fritz Zwicky developed the hypothesis of stars that end their lives in big explosions: supernovae. Only in the 1960s, in a series of three papers by Robert Krafft, the physical nature of novae was explained as surface eruptions on white dwarf stars in cataclysmic binary systems.

2025-09-30T16:59:52Z

← Older revision		Revision as of 16:59, 30 September 2025
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	!Xi and Po<ref>Xi, Ze-Zong, Po, Shu-Jen, Yang, K. S. (1966). Ancient Oriental Records of Novae and Supernovae, Science, Volume 154, Issue 3749, pp. 597-603</ref>		!Xi and Po<ref>Xi, Ze-Zong, Po, Shu-Jen, Yang, K. S. (1966). Ancient Oriental Records of Novae and Supernovae, Science, Volume 154, Issue 3749, pp. 597-603</ref>
	!Hsi 1957<ref>Hsi, T.-T., 1957. "A New Catalog of Ancient Novae", ''Smithonian Contributions to Astrophysics'', Vol. 2, pp. 109-130. [https://ui.adsabs.harvard.edu/abs/1957SCoA....2..109H/abstract adsabs] and [https://articles.adsabs.harvard.edu/full/1957SCoA....2..109H PDF] </ref>		!Hsi 1957<ref>Hsi, T.-T., 1957. "A New Catalog of Ancient Novae", ''Smithonian Contributions to Astrophysics'', Vol. 2, pp. 109-130. [https://ui.adsabs.harvard.edu/abs/1957SCoA....2..109H/abstract adsabs] and [https://articles.adsabs.harvard.edu/full/1957SCoA....2..109H PDF] </ref>
	!Lundmark 1921		!Lundmark 1921<ref>Lundmark (1921). Suspected New Stars Recorded in Old Chronicles and Among Recent Meridian Observations, Publications of the Astronomical Society of the Pacific, Vol. 33, No. 195, p.225

			[https://ui.adsabs.harvard.edu/abs/1921PASP...33..225L/abstract ADSABS]</ref>
	\|-		\|-
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2025-09-30T16:47:43Z

Known Recurrent Novae

2025-07-22T00:31:54Z

← Older revision		Revision as of 00:31, 22 July 2025
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	\|1006		\|1006
	\|Goldstein & Ho (1965)		\|Goldstein & Ho (1965)
	\|		\|G327.6+14.6
	\|		\| -
	\|		\|
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	\|Mayall & Oort (1942)		\|Mayall & Oort (1942)
	\|M1 (Crab N.)		\|M1 (Crab N.)
	\|		\|PSR J0534+2200
	\|		\|
	\|		\|
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	\|1572		\|1572
	\|Baade & Zwicky (1934)		\|Baade & Zwicky (1934)
	\|		\|G120.1+01.4
	\|		\| -
	\|		\|
	\|		\|
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	\|1604		\|1604
	\|Baade (1943)		\|Baade (1943)
	\|		\|G004.5+06.8
	\|		\| -
	\|known asKepler's SN,		\|known asKepler's SN,
	nebula was initally classified a PNcand.		nebula was initally classified a PNcand.

2025-07-22T00:29:57Z

← Older revision		Revision as of 00:29, 22 July 2025
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	!Counterpart		!Counterpart
	Pulsar		Pulsar
			!Commentary
			!Reference
	\|-		\|-
	\|1006		\|1006
			\|Goldstein & Ho (1965)
			\|
	\|		\|
	\|		\|
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	\|-		\|-
	\|1054		\|1054
			\|Mayall & Oort (1942)
			\|M1 (Crab N.)
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	\|-		\|-
	\|1181		\|1181
			\|Stephenson (1971)
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	\|		\|
	\|		\|old identification incorrect
			\|Ritter et al. (2021)
	\|-		\|-
	\|1572		\|1572
			\|Baade & Zwicky (1934)
			\|
	\|		\|
	\|		\|
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	\|-		\|-
	\|1604		\|1604
			\|Baade (1943)
	\|		\|
	\|		\|
			\|known asKepler's SN,
			nebula was initally classified a PNcand.
	\|		\|
	\|}		\|}
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	\|185		\|185
	\|SN		\|SN
	\|Stephenson ()		\|Clarke and Stephenson (1975)
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	\|386		\|386
	\|SN / Nova		\|SN / Nova
	\|		\|Stephenson (1976)
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	\|393		\|393
	\|SN / Nova		\|SN / Nova
	\|		\|Clarke and Stephenson (1975)
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	\|		\|

2025-07-21T22:20:48Z

Suggested Historical Novae or Supernovae

2025-07-21T22:17:18Z

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 Since the dawn of systematic research on variable stars in the 19th century, Sinologists and astrophysicists have attempted to compile catalogues of these objects historically called "nova" (not necessarily implying an underlying nova in the definition of astrophysics) or "guest star".
-== Transients that were suggested as Novae or Supernovae ==
+== Known Stellar Transients ==
 === Known Recurrent Novae ===
@@ Line 167: / Line 167: @@
+|
 |}
 === Compiled List from Authors of the 20th century ===

2024-12-02T09:56:26Z

Compiled List from Authors of the 20th century

2024-12-02T08:38:10Z

Compiled List from Authors of the 20th century: literature reference added

← Older revision		Revision as of 08:38, 2 December 2024
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	!Nikiforov 2010<ref>Nickiforov, Mihael G. (2010). Estimate of the Chinese astronomy development through the descriptions of nova observations, Bulgarian Astronomical Journal, Vol. 13, p. 116</ref>		!Nikiforov 2010<ref>Nickiforov, Mihael G. (2010). Estimate of the Chinese astronomy development through the descriptions of nova observations, Bulgarian Astronomical Journal, Vol. 13, p. 116</ref>
	!Duerbeck 2008?		!Duerbeck 2008?
	!Li Qibin 1988		!Li Qibin 1988<ref>Qibin,Li (1988), A Recent Study on the Historical Novae and Supernovae; In: Börner, G. (eds) High Energy Astrophysics. Springer, Berlin, Heidelberg.

			[https://link.springer.com/chapter/10.1007/978-3-642-73560-8_1 Springer Link] <nowiki>https://doi.org/10.1007/978-3-642-73560-8_1</nowiki></ref>
	!Pskovskii 1972<ref>Pskovskii, Yu. P. (1972). "Survey of Stellar Outbursts of the Pretelescopic Era". ''Soviet Astronomy'', Vol. 16, p. 23.		!Pskovskii 1972<ref>Pskovskii, Yu. P. (1972). "Survey of Stellar Outbursts of the Pretelescopic Era". ''Soviet Astronomy'', Vol. 16, p. 23.

2024-12-02T08:34:17Z

added Qibin column