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19922026
Showing 2021 · astro-ph.SRShow all

14 papers · 2 filters

astro-ph.SR2021★ 41 cited

Helium stars exploding in circumstellar material and the origin of Type Ibn supernovae

Luc Dessart, John Hillier, Hanindyo Kuncarayakti

Type Ibn supernovae (SNe) are a mysterious class of transients whose spectra exhibit persistently narrow HeI lines, and whose bolometric light curves are typically fast evolving an…

astro-ph.SR2021★ 13 cited

The Physical Parameters of Four WC-type Wolf-Rayet Stars in the Large Magellanic Cloud: Evidence of Evolution

Erin Aadland, Philip Massey, D. John Hillier +1

We present a spectral analysis of four LMC WC-type Wolf-Rayet (WR) stars (BAT99-8, BAT99-9, BAT99-11, and BAT99-52) to shed light on two evolutionary questions surrounding massive…

astro-ph.SR2021

Stellar multiplicity and stellar rotation: Insights from APOGEE

Christine Mazzola Daher, Carles Badenes, Jamie Tayar +18

We measure rotational broadening in spectra taken by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey to characterise the relationship between stellar mul…

astro-ph.SR2021★ 48 cited

Nebular phase properties of supernova Ibc from He-star explosions

L. Dessart, D. J. Hillier, T. Sukhbold +2

Following our recent work on Type II supernovae (SNe), we present a set of 1D nonlocal thermodynamic equilibrium radiative transfer calculations for nebular-phase Type Ibc SNe star…

astro-ph.SR2021★ 34 cited

Stable nickel production in Type Ia supernovae: A smoking gun for the progenitor mass?

Stéphane Blondin, Eduardo Bravo, Frank Timmes +2

At present, there are strong indications that white dwarf (WD) stars with masses well below the Chandrasekhar limit (MCh ~ 1.4 Msun) contribute a significant fraction of SN Ia prog…

astro-ph.SR2021★ 16 cited

A 99-minute Double-lined White Dwarf Binary from SDSS-V

Vedant Chandra, Hsiang-Chih Hwang, Nadia L. Zakamska +12

We report the discovery of SDSS J133725.26+395237.7 (hereafter SDSS J1337+3952), a double-lined white dwarf (WD+WD) binary identified in early data from the fifth generation Sloan…