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Roseanne M. Cheng

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • gr-qc1
ORCID 0000-0002-4854-8636

identity via Semantic Scholar / OpenAlex

most citedGeneral Relativistic Hydrodynamic Simulation of Accretion Flow from a Stellar Tidal Disruption

320 citations · 374 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2015★ 6 cited

"Circularization" vs. Accretion -- What Powers Tidal Disruption Events?

Tsvi Piran, Gilad Svirski, Julian Krolik +2

A tidal disruption event (TDE) takes place when a star passes near enough to a massive black hole to be disrupted. About half the star's matter is given elliptical trajectories wit…

astro-ph.HE2015★ 320 cited

General Relativistic Hydrodynamic Simulation of Accretion Flow from a Stellar Tidal Disruption

Hotaka Shiokawa, Julian H. Krolik, Roseanne M. Cheng +2

We study how the matter dispersed when a supermassive black hole tidally disrupts a star joins an accretion flow. Combining a relativistic hydrodynamic simulation of the stellar di…

gr-qc2014★ 48 cited

Tidal disruption of a star in the Schwarzschild spacetime: relativistic effects in the return rate of debris

Roseanne M. Cheng, Tamara Bogdanovic

Motivated by an improved multi-wavelength observational coverage of the transient sky, we investigate the importance of relativistic effects in disruptions of stars by non-spinning…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.