activity
20182026
most citedCharacterizing the continuous gravitational-wave signal from boson clouds around Galactic isolated black holes

107 citations · 785 across the 63 of their papers we have counts for

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Showing 2024Show all

12 papers · 1 filter

astro-ph.HE2024★ 2 cited

Dinosaur in a Haystack : X-ray View of the Entrails of SN 2023ixf and the Radio Afterglow of Its Interaction with the Medium Spawned by the Progenitor Star (Paper 1)

A. J. Nayana, Raffaella Margutti, Eli Wiston +24

We present the results from our extensive hard-to-soft X-ray (NuSTAR, Swift-XRT, XMM-Newton, Chandra) and meter-to-mm wave radio (GMRT, VLA, NOEMA) monitoring campaign of the very…

astro-ph.HE2024

Transients by Black Hole Formation from Red Supergiants: Impact of Dense Circumstellar Matter

Daichi Tsuna, Xiaoshan Huang, Jim Fuller +1

Failed supernovae (SNe), which are likely the main channel for forming stellar-mass black holes, are predicted to accompany mass ejections much weaker than typical core-collapse SN…

astro-ph.HE2024★ 17 cited

A cosmic formation site of silicon and sulphur revealed by a new type of supernova explosion

Steve Schulze, Avishay Gal-Yam, Luc Dessart +47

The cores of stars are the cosmic furnaces where light elements are fused into heavier nuclei. The fusion of hydrogen to helium initially powers all stars. The ashes of the fusion…

astro-ph.HE2024

The X-ray Luminous Type Ibn SN 2022ablq: Estimates of Pre-explosion Mass Loss and Constraints on Precursor Emission

C. Pellegrino, M. Modjaz, Y. Takei +14

Type Ibn supernovae (SNe Ibn) are rare stellar explosions powered primarily by interaction between the SN ejecta and H-poor, He-rich material lost by their progenitor stars. Multi-…

astro-ph.SR2024★ 36 cited

Boil-off of red supergiants: mass loss and type II-P supernovae

Jim Fuller, Daichi Tsuna

The mass loss mechanism of red supergiant stars is not well understood, even though it has crucial consequences for their stellar evolution and the appearance of supernovae that oc…

astro-ph.HE2024★ 15 cited

Merger Precursor: Year-long Transients Preceding Mergers of Low-mass Stripped Stars with Compact Objects

Daichi Tsuna, Samantha C. Wu, Jim Fuller +2

Binary mass transfer can occur at high rates due to rapid expansion of the donor's envelope. In the case where mass transfer is unstable, the binary can rapidly shrink its orbit an…