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| Query : 2007Natur.450..390W |
2007Natur.450..390W - Nature, 450, 390-392 (2007)
Pulsational pair instability as an explanation for the most luminous supernovae.
WOOSLEY S.E., BLINNIKOV S. and HEGER A.
Journal keyword(s):
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | SN 2006gy | SN* | 03 17 27.06 | +41 24 19.5 | 14.20 | SNIIn | 372 | 1 | ||||
| 2 | SN 1994W | SN* | 12 02 10.92 | +62 08 32.7 | 13.3 | SNIInP | 194 | 1 |
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