activity
20022026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 8.3k across the 160 of their papers we have counts for

collaborators
Showing 2021Show all

8 papers · 1 filter

astro-ph.SR2021★ 20 cited

The dawn of a new era for dustless HdC stars with GAIA eDR3

P. Tisserand, C. L. Crawford, G. C. Clayton +7

Decades after their discovery, only four hydrogen-deficient carbon (HdC) stars were known to have no circumstellar dust shell. This is in complete contrast to the 130 known G…

astro-ph.HE2021★ 14 cited

Forbidden Line Emission from Type Ia Supernova Remnants Containing Balmer-Dominated Shells

Chuan-Jui Li, You-Hua Chu, John C. Raymond +3

Balmer-dominated shells in supernova remnants (SNRs) are produced by collisionless shocks advancing into a partially neutral medium, and are most frequently associated with Type Ia…

astro-ph.GA2021★ 24 cited

First extragalactic measurement of the turbulence driving parameter: ALMA observations of the star-forming region N159E in the Large Magellanic Cloud

Piyush Sharda, Shyam H. Menon, Christoph Federrath +13

Studying the driving modes of turbulence is important for characterizing the impact of turbulence in various astrophysical environments. The driving mode of turbulence is parameter…

astro-ph.HE2021★ 11 cited

Type Ia Supernova Models: Asymmetric Remnants and Supernova Remnant G1.9+0.3

Alice G. Stone, Heather T. Johnson, John M. Blondin +5

The youngest Galactic supernova remnant G1.9+0.3, probably the result of a Type Ia supernova, shows surprising anomalies in the distribution of its ejecta in space and velocity. In…

astro-ph.HE2021★ 10 cited

SN 2018bsz: significant dust formation in a nearby superluminous supernova

T. -W. Chen, S. J. Brennan, R. Wesson +41

We investigate the thermal emission and the extinction from dust associated with the nearby (z = 0.0267) superluminous supernova (SLSN) 2018bsz. Our dataset combines daily-cadence,…

astro-ph.SR2021★ 3 cited

Searching for Surviving Companion in the Young SMC Supernova Remnant 1E 0102.2-7219

Chuan-Jui Li, Ivo R. Seitenzahl, Ryoko Ishioka +3

1E 0102.2--7219 (hereafter E0102) is a young supernova remnant (SNR) in the Small Magellanic Cloud (SMC). It contains oxygen-rich SN ejecta, a possible neutron star (NS), and a sma…

astro-ph.HE2021★ 7 cited

Prospects of direct detection of V gamma-rays from thermonuclear supernovae

Fiona H. Panther, Ivo R. Seitenzahl, Ashley J. Ruiter +3

Detection of gamma-rays emitted by radioactive isotopes synthesized in stellar explosions can give important insights into the processes that power transients such as supernovae, a…

astro-ph.HE2021★ 50 cited

Metallicity-dependent nucleosynthetic yields of Type Ia supernovae originating from double detonations of sub-M white dwarfs

Sabrina Gronow, Benoit Cote, Florian Lach +4

Double detonations in sub-Chandrasekhar mass carbon-oxygen white dwarfs with helium shell are a potential explosion mechanism for a Type Ia supernova (SNe Ia). It comprises a shell…