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20112026
most citedA long-lived remnant neutron star after GW170817 inferred from its associated kilonova

127 citations · 974 across the 44 of their papers we have counts for

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Showing 2021Show all

7 papers · 1 filter

astro-ph.SR2021★ 34 cited

An environmental analysis of the Type Ib SN 2019yvr and the possible presence of an inflated binary companion

Ning-Chen Sun, Justyn R. Maund, Paul A. Crowther +5

SN 2019yvr is the second Type Ib supernova (SN) with a possible direct detection of its progenitor (system); however, the spectral energy distribution (SED) of the pre-explosion so…

astro-ph.HE2021★ 13 cited

Searching for gravitationally lensed gamma-ray bursts with their afterglows

Sheng-Nan Chen, Xu-Dong Wen, He Gao +8

Gamma-ray bursts (GRBs) at high redshifts are expected to be gravitationally lensed by objects of different mass scales. Besides a single recent claim, no lensed GRB has been detec…

astro-ph.SR2021★ 20 cited

Error Analysis of the Light Curve Solution of Contact Binaries Based on the W-D Code

Liang Liu

We use the idea of repeat measurement to determine the mean value and error of light curve solution parameters of contact binaries. Our simulation is realized by the Monte Carlo al…

astro-ph.HE2021★ 49 cited

No Detectable Kilonova Counterpart is Expected for O3 Neutron Star-Black Hole Candidates

Jin-Ping Zhu, Shichao Wu, Yuan-Pei Yang +5

We analyse the tidal disruption probability of potential neutron star--black hole (NSBH) merger gravitational wave (GW) events, including GW190426_152155, GW190814, GW200105_162426…

astro-ph.HE2021★ 37 cited

Thermonuclear Explosions and Accretion-induced Collapses of White Dwarfs in Active Galactic Nucleus Accretion Disks

Jin-Ping Zhu, Yuan-Pei Yang, Bing Zhang +3

White dwarfs (WDs) embedded in gaseous disks of active galactic nucleus (AGNs) can rapidly accrete materials from the disks and grow in mass to reach or even exceed the Chandrasekh…

astro-ph.SR2021★ 4 cited

The Deep and Low-Mass-Ratio Contact Binary CSS J022914.4+044340 with A Luminous Additional Companion

Liang Liu, Xu-Zhi Li

The first B-, V-, Rc-, and Ic-band light curves of CSS J022914.4+044340 are presented and analyzed. It is found that CSS J022914.4+044340 is a low mass ratio (0.198 +- 0.005) deep…

astro-ph.HE2021★ 16 cited

Magnetar-Driven Shock Breakout Revisited and Implications for Double-Peaked Type I Superluminous Supernovae

Liang-Duan Liu, He Gao, Xiao-Feng Wang +1

The discovery of early bumps in some type-I superluminous supernovae (SLSNe-I) before the main peaks offers an important clue to their energy source mechanisms. In this paper, we u…