Panning for gold, but finding helium: Discovery of the ultra-stripped supernova SN 2019wxt from gravitational-wave follow-up observations
Journal article, 2023

We present the results from multi-wavelength observations of a transient discovered during an intensive follow-up campaign of S191213g, a gravitational wave (GW) event reported by the LIGO-Virgo Collaboration as a possible binary neutron star merger in a low latency search. This search yielded SN 2019wxt, a young transient in a galaxy whose sky position (in the 80% GW contour) and distance (∼150 Mpc) were plausibly compatible with the localisation uncertainty of the GW event. Initially, the transienta's tightly constrained age, its relatively faint peak magnitude (Mi ∼ -16.7 mag), and the r-band decline rate of ∼1 mag per 5 days appeared suggestive of a compact binary merger. However, SN 2019wxt spectroscopically resembled a type Ib supernova, and analysis of the optical-near-infrared evolution rapidly led to the conclusion that while it could not be associated with S191213g, it nevertheless represented an extreme outcome of stellar evolution. By modelling the light curve, we estimated an ejecta mass of only ∼0.1 M·, with 56Ni comprising ∼20% of this. We were broadly able to reproduce its spectral evolution with a composition dominated by helium and oxygen, with trace amounts of calcium. We considered various progenitor channels that could give rise to the observed properties of SN 2019wxt and concluded that an ultra-stripped origin in a binary system is the most likely explanation. Disentangling genuine electromagnetic counterparts to GW events from transients such as SN 2019wxt soon after discovery is challenging: in a bid to characterise this level of contamination, we estimated the rate of events with a volumetric rate density comparable to that of SN 2019wxt and found that around one such event per week can occur within the typical GW localisation area of O4 alerts out to a luminosity distance of 500 Mpc, beyond which it would become fainter than the typical depth of current electromagnetic follow-up campaigns.

Gravitational waves

Supernovae: individual: SN2019wxt

Binaries: general

Stars: evolution

Supernovae: general

Author

I. Agudo

Institute of Astrophysics of Andalusia (IAA)

L. Amati

Istituto nazionale di astrofisica (INAF)

T. An

Shanghai Astronomical Observatory

F. E. Bauer

Pontificia Universidad Catolica de Chile

S. Benetti

Istituto nazionale di astrofisica (INAF)

M.G. Bernardini

Istituto nazionale di astrofisica (INAF)

R. J. Beswick

University of Manchester

K. Bhirombhakdi

Space Telescope Science Institute (STScI)

T. De Boer

University of Hawaii

M. Branchesi

Gran Sasso Science Institute (GSSI)

S.J. Brennan

University College Dublin

E. Brocato

Istituto nazionale di astrofisica (INAF)

M.D. Caballero-García

Institute of Astrophysics of Andalusia (IAA)

E. Cappellaro

Istituto nazionale di astrofisica (INAF)

N. Castro Rodríguez

Instituto de Astrofísica de Canarias

A.J. Castro-Tirado

Institute of Astrophysics of Andalusia (IAA)

K.C. Chambers

University of Hawaii

E. Chassande-Mottin

APC - AstroParticule et Cosmologie

S. Chaty

APC - AstroParticule et Cosmologie

T.-W. Chen

Oskar Klein Centre

A. Coleiro

APC - AstroParticule et Cosmologie

S. Covino

Istituto nazionale di astrofisica (INAF)

F. Da'ammando

Istituto di Radioastronomia

P. Da'avanzo

Istituto nazionale di astrofisica (INAF)

V. Da'elia

Osservatorio Astronomico di Roma

A. Fiore

Istituto nazionale di astrofisica (INAF)

A. Flörs

Helmholtz

M Fraser

University College Dublin

S. Frey

Hungarian Academy of Sciences

C. Frohmaier

University of Southampton

M. Fulton

Queen's University Belfast

L. Galbany

Institute of Space Sciences (ICE) - CSIC

C. Gall

Niels Bohr Institute

H. Gao

University of Hawaii

Jorge García-Rojas

Instituto de Astrofísica de Canarias

G. Ghirlanda

Istituto nazionale di astrofisica (INAF)

S. Giarratana

Istituto di Radioastronomia

J.H. Gillanders

Queen's University Belfast

M. Giroletti

Istituto di Radioastronomia

B.P. Gompertz

University of Birmingham

M. Gromadzki

University of Warsaw

K. E. Heintz

Cosmic Dawn Center (DAWN)

J. Hjorth

Niels Bohr Institute

Y.-D. Hu

Institute of Astrophysics of Andalusia (IAA)

M.E. Huber

University of Hawaii

A. Inkenhaag

Radboud University

L. Izzo

Niels Bohr Institute

Z.P. Jin

Chinese Academy of Sciences

P. G. Jonker

Radboud University

D.A. Kann

Institute of Astrophysics of Andalusia (IAA)

E.C. Kool

Oskar Klein Centre

R Kotak

University of Turku

G. Leloudas

Technical University of Denmark (DTU)

Andrew Levan

Radboud University

C. C. Lin

University of Hawaii

J.D. Lyman

The University of Warwick

E.A. Magnier

University of Hawaii

K. Maguire

Trinity College Dublin

I. Mandel

Monash University

B. Marcote

Joint Institute for VLBI in Europe (JIVE)

D. Mata Sánchez

Instituto de Astrofísica de Canarias

S. Mattila

University of Turku

A. Melandri

Istituto nazionale di astrofisica (INAF)

M.J. Michaåà  Owski

Adam Mickiewicz University in Poznań

J. Moldon

Institute of Astrophysics of Andalusia (IAA)

M. Nicholl

University of Birmingham

A. Nicuesa Guelbenzu

Thüringer Landessternwarte Tautenburg

S.R. Oates

University of Birmingham

F. Onori

Istituto nazionale di astrofisica (INAF)

M. Orienti

Istituto di Radioastronomia

R. Paladino

Istituto di Radioastronomia

Z. Paragi

Joint Institute for VLBI in Europe (JIVE)

M.A. Pérez-Torres

Institute of Astrophysics of Andalusia (IAA)

E. Pian

Istituto nazionale di astrofisica (INAF)

G. Pignata

Millennium Institute of Astrophysics

S. Piranomonte

Osservatorio Astronomico di Roma

J. Quirola-Vásquez

Pontificia Universidad Catolica de Chile

F. Ragosta

Osservatorio Astronomico di Roma

A. Rau

Max Planck Society

S. Ronchini

Gran Sasso Science Institute (GSSI)

A. Rossi

Istituto nazionale di astrofisica (INAF)

R. Sánchez-Ramírez

Institute of Astrophysics of Andalusia (IAA)

O. S. Salafia

Istituto nazionale di astrofisica (INAF)

S. Schulze

Oskar Klein Centre

S. J. Smartt

Queen's University Belfast

K.W. Smith

Queen's University Belfast

J Sollerman

Oskar Klein Centre

S. Srivastav

Queen's University Belfast

R. L. C. Starling

University Of Leicester

D. Steeghs

The University of Warwick

H.F. Stevance

Queen's University Belfast

Nial R. Tanvir

University Of Leicester

Vincenzo Testa

Osservatorio Astronomico di Roma

M.A.P. Torres

Instituto de Astrofísica de Canarias

A. Valeev

Russian Academy of Sciences

S. D. Vergani

Observatoire de Paris-Meudon

D. Vescovi

Goethe University Frankfurt

R. Wainscost

University of Hawaii

D. Watson

Cosmic Dawn Center (DAWN)

K. Wiersema

The University of Warwick

Lukasz Wyrzykowski

University of Warsaw

Jun Yang

Chalmers, Space, Earth and Environment, Onsala Space Observatory

S. Yang

Oskar Klein Centre

D.R. Young

Queen's University Belfast

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 675 A201

Subject Categories

Astronomy, Astrophysics and Cosmology

DOI

10.1051/0004-6361/202244751

More information

Latest update

10/10/2023