SN 1997D
This article includes a list of references, related reading, or external links, but its sources remain unclear because it lacks inline citations. (May 2022) |
| File:SN 1997D.jpg Lua error in Module:Wikidata at line 800: attempt to index field 'wikibase' (a nil value). | |
| Other designations | Lua error in Module:Wikidata at line 448: attempt to index field 'wikibase' (a nil value). |
|---|---|
| Website | <strong%20class= "error"><span%20class="scribunto-error%20mw-scribunto-error-1eb9e9c4">Lua%20error%20in%20Module:Wikidata%20at%20line%20448:%20attempt%20to%20index%20field%20'wikibase'%20(a%20nil%20value). http://<strong%20class="error"><span%20class="scribunto-error%20mw-scribunto-error-1eb9e9c4">Lua%20error%20in%20Module:Wikidata%20at%20line%20448:%20attempt%20to%20index%20field%20'wikibase'%20(a%20nil%20value). |
| Error creating thumbnail: File missing Lua error in Module:Commons_link at line 62: attempt to index field 'wikibase' (a nil value). | |
SN 1997D, discovered in January 1997 by Duília de Mello in galaxy NGC 1536 in Reticulum constellation is a first clearly identified example of atypical Type II supernova with a very low luminosity and expansion velocity.
Progenitor
[edit | edit source]There are two alternatives, a high-mass 25-40 solar masses star or smaller star with mass of 8-10 solar masses. As there is no evidence that neutron star was formed during the collapse of the star, it is likely that star was in upper spectrum of the mass.
Remnants
[edit | edit source]Observations of the light curve from SN 1997D showed no evidence of other energy sources in the expanding supernova envelope therefore it is unlikely that a Neutron star was created, all the evidence leads to the creation of the stellar mass black hole of approximately 3 solar masses.
