2022RAA....22e5010S


Query : 2022RAA....22e5010S

2022RAA....22e5010S - Research in Astron. and astroph., 22, part no 5, 5010-5010 (2022/May-~)

A Common Envelope Jets Supernova (CEJSN) Impostor Scenario for Fast Blue Optical Transients.

SOKER N.

Abstract (from CDS):

I propose a new scenario, the polar common envelope jets supernova (CEJSN) impostor scenario, to account for AT2018cow-like fast blue optical transients (FBOTs). The polar CEJSN impostor scenario evolves through four main phases. (1) A red supergiant (RSG) star expands to tidally interact with a neutron star (NS) companion (or a black hole). The interaction increases the RSG mass loss rate to form a circumstellar matter (CSM) halo to r ≃ 0.1 pc. (2) Shortly before the onset of a common envelope evolution (CEE) and about a year before explosion the NS accretes mass from the RSG envelope and launches jets that inflate two opposite lobes in the CSM within ≃100 au. (3) The NS-RSG system enters a CEE phase during which the system ejects most of the envelope mass in a dense equatorial outflow. (4) At the termination of the CEE the leftover envelope forms a circumbinary disk around the NS-core system. The NS accretes mass from the circumbinary disk and launches energetic jets that, when colliding with the fronts of the CSM lobes, power an FBOT event. The low mass of the jets-lobes interaction zones and their large distance, of about 100 au, from the center account for the fast transient. In the future the core collapses to form a second NS. In the far future the two NSs might merge. I suggest that FBOTs and similar fast transients are CEJSN impostors which compose a large fraction of the progenitors of NS-NS merger binaries.

Abstract Copyright: © 2022. National Astronomical Observatories

Journal keyword(s): neutron stars - supernovae - stellar jets - common envelope binary stars - transient sources

Simbad objects: 14

goto Full paper

goto View the references in ADS

Number of rows : 14
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 GRB 101225A gB 00 00 47.48 +44 36 01.0           ~ 163 0
2 AT 2018lug ev 02 00 15.19 +16 47 57.3           ~ 54 0
3 CRTS CSS161010 J045834-081803 ev 04 58 34.0 -08 18 03           ~ 35 0
4 HD 44179 pA* 06 19 58.2185496 -10 38 14.706068 9.51 9.33 9.02     B9Ib/II 800 0
5 SN 2016bse SN* 09 20 34.30 +50 41 46.8           SNIIP 134 0
6 NAME Homunculus Nebula ISM 10 45 03.5 -59 41 04           ~ 379 1
7 * eta Car s*b 10 45 03.545808 -59 41 03.95124 6.37 7.03 6.48 6.123 4.41 LBV 2543 0
8 M 97 PN 11 14 47.7122947800 +55 01 08.482832076   15.414 15.777 15.960 16.194 ~ 356 2
9 VT J121001+495647 Rad 12 10 01.32 +49 56 46.9           ~ 14 0
10 SN 2020faa SN* 14 47 09.469 +72 44 11.56           SNII 22 0
11 SN 2020mrf SN* 15 47 54.163 +44 39 07.41           SNII 37 0
12 AT 2018lqh ev 16 06 04.470 +36 52 16.50           ~ 10 0
13 SN 2018cow SN* 16 16 00.254 +22 16 05.10           SNIb 305 0
14 AT 2020xnd ev 22 20 02.030 -02 50 25.30           ~ 66 0

To bookmark this query, right click on this link: simbad:objects in 2022RAA....22e5010S and select 'bookmark this link' or equivalent in the popup menu