Ушбу ишга иқтибос қилган ишлар

3 та иш

Иш: 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

   МақолаAstrophysical Phenomena and ObservationsNew Astronomy202217 иқтибос

   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

   МақолаAstrophysical Phenomena and ObservationsMonthly Notices of the Royal Astronomical Society20230 иқтибос

   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)20230 иқтибос

   ABIABI:AkademIndex/openalex/2023.preprint.000158