2025ApJ...982L..55L


Query : 2025ApJ...982L..55L

2025ApJ...982L..55L - Astrophys. J., 982, L55 (2025/April-1)

The Red Supergiant Progenitor of the Type II Supernova 2024abfl.

LUO J., ZHANG L., CHEN B.-Q., CHENG Q., GUO B., LI J., GUO Y., XIONG J., MENG X., CHEN X., LIU Z. and HAN Z.

Abstract (from CDS):

Linkage between core-collapse supernovae and their progenitors is not fully understood and ongoing effort of searching and identifying the progenitors is needed. SN 2024abfl is a recent Type II supernova that exploded in the nearby star-bursting galaxy NGC 2146, which is also the host galaxy of SN 2018zd. From archival Hubble Space Telescope data, we have found a red source (mF814W ∼ 25) near the location (angular distance ≤0$\mathop{.}\limits^{\unicode{x02033}}$2) of SN 2024abfl before its explosion. With F814W and F606W photometry, we found that the properties of this source matched a typical red supergiant (RSG) moderately reddened by interstellar dust at the distance of the host galaxy. We conclude that the SN 2024abfl had an RSG progenitor with initial mass of 9 -12 M⊙.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Stellar evolution - Type II supernovae - Red supergiant stars

Simbad objects: 6

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Number of rows : 6
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 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
2 * alf Ori s*r 05 55 10.30536 +07 24 25.4304 4.38 2.27 0.42 -1.17 -2.45 M1-M2Ia-Iab 1789 0
3 SN 2024abfl SN* 06 18 01.140 +78 22 01.52           SNII 1 0
4 SN 2018zd SN* 06 18 03.180 +78 22 00.90           SNII 74 0
5 NGC 2146 AGN 06 18 37.710 +78 21 25.27 11.67 11.38 10.59     ~ 765 2
6 SN 2023ixf SN* 14 03 38.562 +54 18 41.94           SNII 209 0

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