2024AstBu..79..210T


Query : 2024AstBu..79..210T

2024AstBu..79..210T - Astrophys. Bull., 79, 210-210 (2024/April-0)

SN 2022prv: Bright Type-II Supernova with Signs of Interaction with Circumstellar Matter

TSVETKOV D.Y., GORANSKY V.P., BARSUKOVA E.A., VALEEV A.F., PAVLYUK N.N., DODIN A.V., SHATSKY N.I., POTANIN S.A., IKONNIKOVA N.P., BURLAK M.A., BELINSKY A.A., ECHEISTOV V.A., VINOKUROV A.S., SARKISYAN A.N. and ZHAROVA A.V.

Abstract (from CDS):

The results of photometric and spectroscopic observations of supernova SN 2022prv carried out with six telescopes including the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences and the 2.5-m telescope of the Caucasus Mountain Observatory of SAI MSU are presented. The dates and magnitudes at the brightness maximum and the parameters of the light curves are determined. The photometric evolution of SN 2022prv is characterized by a constant decrease in brightness after the maximum at a rate quite high for a type II supernovae. Approximately 55 days after the maximum, the rate of the decrease in brightness increased. The maximum luminosity has reached M_V=-18.1 which is higher than average for SN II. In the pre-maximum spectra, high-excitation emission lines were observed characteristic of the ionization of the circumstellar matter by a burst during the shock wave emergence onto the surface of the star. However, approximately 20 days after the maximum, the spectrum did not differ from that typical of SN II. The rate of the envelope expansion at this stage was about 3500 km/s

Abstract Copyright: ∼

Journal keyword(s): supernovae: individual: SN 2022prv

Simbad objects: 1

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Number of rows : 1
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 AT 2022prv SN? 15 40 07.750 +20 40 31.78           SNII 6 0

Query : 2024AstBu..79..210T

Basic data :
AT 2022prv -- SuperNova Candidate
Other object types:
otypes_help
ev (AT,PSST), SN* (SN), SN? (2022ATel15530)
ICRS coord. (ep=J2000) :
15 40 07.750 +20 40 31.78 [ ] D 2022ATel15530....1T
FK4 coord. (ep=B1950 eq=1950) :
15 37 54.655 +20 50 10.05 [ ]
Gal coord. (ep=J2000) :
032.754700 +51.087518 [ ]
Radial velocity / Redshift / cz :
V(km/s) 4493 [~] / z(~) 0.015101 [~] / cz 4527.17 [~]
   D 2022ATel15530....1T
Spectral type:
SNII C 2022ATel15530....1T
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Hierarchy : number of linked objects
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: 1 : 65 Display criteria :

Identifiers (3) :
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SN 2022prv AT 2022prv PSST 22gjh

References (6 between 1850 and 2026) (Total 6)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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