Работы, цитирующие эту работу

Работ: 3

Работа: Optical Observations of GRO J1655−40 in Quiescence. I. A Precise Mass for the Black Hole Primary

1. Regular black hole solution in PFDM environment to explain the radiative efficiency of black hole candidates

   Bakhtiyor Narzilloev, Bobomurat Ahmedov

   СтатьяAstrophysical Phenomena and ObservationsNew Astronomy2022Цитирований: 17

   ABIABI:AkademIndex/openalex/2026.other.088292

2. Measuring black hole spins through X-ray reflection spectroscopy and the relativistic precession model: the case of XTE J1859+226

   Gitika Mall, H. Liu, Cosimo Bambi +2

   СтатьяAstrophysical Phenomena and ObservationsMonthly Notices of the Royal Astronomical Society2023Цитирований: 0

   ABIABI:AkademIndex/openalex/2023.article.000831

3. Measuring Black Hole Spins through X-ray Reflection Spectroscopy and the Relativistic Precession Model: the case of XTE J1859+226

   Gitika Mall, H. Liu, Cosimo Bambi +2

   ПрепринтAstrophysical Phenomena and ObservationsarXiv (Cornell University)2023Цитирований: 0

   ABIABI:AkademIndex/openalex/2023.preprint.000158