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20082026
most citedDynamics and Gravitational Wave Signature of Collapsar Formation

136 citations · 405 across the 12 of their papers we have counts for

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9 papers · 1 filter

astro-ph.HE2026

Parameter Estimation Horizon of Core-Collapse Supernovae with a Network of Gravitational-Wave Detectors

Almat Akhmetali, Y. Sultan Abylkairov, Solange Nunes +3

Core-collapse supernovae are among the most promising yet still undetected sources of gravitational waves. A future detection would provide a direct view of the physical processes…

astro-ph.GA2026

Centrally concentrated star formation in young clusters II: Jet feedback

Adilkhan Assilkhan, Sabrina M. Appel, Bekdaulet Shukirgaliyev +5

Protostellar jets are one of the earliest forms of stellar feedback, but their impact on star formation and cluster assembly in centrally concentrated molecular clouds remains poor…

astro-ph.HE2026

Earliest simultaneous multi-color optical observations of GRB 230328B: from 41 seconds to the host-galaxy identification

T. Komesh, A. Pozanenko, N. Pankov +36

We present a multiwavelength study of the long-duration gamma-ray burst GRB 230328B, combining prompt gamma-ray observations with exceptionally early simultaneous optical photometr…

astro-ph.HE2026

Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors

Almat Akhmetali, Y. Sultan Abylkairov, Daniil Orel +7

Core-collapse supernovae (CCSNe) are powerful sources of gravitational waves (GWs). These signals propagate essentially unobstructed, providing a unique probe of the supernova cent…

astro-ph.HE2026

A fast X-ray transient with chromatic flares: signatures of violent collisions induced by late-time central engine reactivation

Shao-Yu Fu, Cui-Yuan Dai, Ai-Ling Wang +57

Extragalactic Fast X-ray Transients (EFXTs) represent an emerging class of high-energy phenomena characterized by X-ray outbursts lasting from tens to hundreds of seconds. However,…

astro-ph.HE2026

Systematic Study of Forward and Reverse Shock Afterglow Emission from Two-Component Jets

Olzhas Mukazhanov, Ernazar Abdikamalov, Paz Beniamini

Two-component jets are frequently invoked to explain complex features in gamma-ray burst (GRB) afterglows, such as late-time rebrightening and chromatic breaks. While many studies…