SIMBAD references

2020ApJ...890..159L - Astrophys. J., 890, 159-159 (2020/February-3)

The deepest radio observations of nearby SNe Ia: constraining progenitor types and optimizing future surveys.

LUNDQVIST P., KUNDU E., PEREZ-TORRES M.A., RYDER S.D., BJORNSSON C.-I., MOLDON J., ARGO M.K., BESWICK R.J., ALBERDI A. and KOOL E.C.

Abstract (from CDS):

We report deep radio observations of nearby Type Ia supernovae (SNe Ia) with the electronic Multi-Element Radio Linked Interferometer Network and the Australia Telescope Compact Array. No detections were made. With standard assumptions for the energy densities of relativistic electrons going into a power-law energy distribution and the magnetic field strength (εe = εB = 0.1), we arrive at upper limits on mass-loss rate for the progenitor system of SN 2013dy (SN 2016coj, SN 2018gv, SN 2018pv, SN 2019np) of {dot}M≲12(2.8,1.3,2.1,1.7)×10–8Myr–1(vw/100kms–1), where vw is the wind speed of the mass loss. To SN 2016coj, SN 2018gv, SN 2018pv, and SN 2019np we add radio data for 17 other nearby SNe Ia and model their nondetections. With the same model as described, all 21 SNe Ia have {dot}M≲4×10–8Myr–1(vw/100kms–1). We compare those limits with the expected mass-loss rates in different single-degenerate progenitor scenarios. We also discuss how information on εe and εB can be obtained from late observations of SNe Ia and the youngest SN Ia remnant detected in radio, G1.9+0.3, as well as stripped-envelope core-collapse SNe. We highlight SN 2011dh and argue for εe ≃ 0.1 and εB ≃ 0.0033. Finally, we discuss strategies to observe at radio frequencies to maximize the chance of detection, given the time since explosion, the distance to the SN, and the telescope sensitivity.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Supernova remnants - Type Ia supernovae - White dwarf stars - Stellar mass loss - Radio continuum emission

Simbad objects: 63

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2020ApJ...890..159L and select 'bookmark this link' or equivalent in the popup menu


2021.06.19-20:44:46

© Université de Strasbourg/CNRS

    • Contact