| Name: | Devendra Sahu |
| Affiliation: | Indian Institute of Astrophysics |
| Conference ID : | ASI2024_944 |
| Title : | Photometric and Spectroscopic Studies of Supernova SN 2021mxx |
| Authors : | D.K. Sahu1, Mulchand Kurre2, G.C. Anupama1, Yogita Patel2, N.K. Chakradhari3 |
| Authors Affiliation: | 1 D.K. Sahu, G.C. Anupama (Indian Institute of Astrophysics, Bangalore - 560034, India)
2 Mulchand Kurre, Yogita Patel (CREST Campus, Indian Institute of Astrophysics, Hoskote - 562114, India)
3 N.K. Chakradhari (Pt. Ravishankar Shukla University, Raipur - 492010, India) |
| Mode of Presentation: | Poster |
| Abstract Category : | High Energy Phenomena, Fundamental Physics and Astronomy |
| Abstract : | We present detailed analysis of supernova SN 2021mxx in the galaxy UGC11380. Our observations covered evolution of this supernova from -2.4 to +115 days with respect to the epoch of peak brightness in B band. SN 2021mxx reached its maximum brightness in the B band, with an apparent magnitude of 16.91 ± 0.03 mag on JD 2459363. The peak absolute B band magnitude and peak quasi-bolometric luminosity of this supernova are estimated as -16.70 ± 0.2 mag and log L = 42.30 +/- 0.06 erg/sec, respectively. Though this supernova was initially classified as Type Ia, the combined photometric and spectroscopic analyses suggest that SN 2021mxx exhibits characteristics typical of a normal Type-Ic supernova. |
