G. R. Bhuvana

most citedRevealing the nature of the transient source MAXI J0637-430 through spectro-temporal analysis

17 citations · 17 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.HE2026

An ALMA view of the Jet-Arc CO clouds toward the TeV $γ$ -ray source HESS J1023-575 and Westerlund 2; Evidence for the footprints of microquasar jets, the very powerful cosmic-ray accelerator in the Galactic disk

Yasuo Fukui, Kisetsu Tsuge, Hidetoshi Sano +7

The TeV $γ$ -ray source HESS J1023-575 (HESSJ 1023 hereafter) is one of the brightest H.E.S.S. sources near the young massive cluster Westerlund 2. HESS J1023 shows a remarkable pos…

astro-ph.HE2021★ 17 cited

Revealing the nature of the transient source MAXI J0637-430 through spectro-temporal analysis

Blessy E. Baby, Bhuvana G. R., Radhika D. +3

We study the spectral and temporal properties of MAXI J0637-430 during its 2019-2020 outburst using \textit{NICER}, \textit{AstroSat} and \textit{Swift-XRT} data. The source was in…

An ALMA view of the Jet-Arc CO clouds toward the TeV γ-ray source HESS J1023-575 and Westerlund 2; Evidence for the footprints of microquasar jets, the very powerful cosmic-ray accelerator in the Galactic disk

Revealing the nature of the transient source MAXI J0637-430 through spectro-temporal analysis

An ALMA view of the Jet-Arc CO clouds toward the TeV $γ$ -ray source HESS J1023-575 and Westerlund 2; Evidence for the footprints of microquasar jets, the very powerful cosmic-ray accelerator in the Galactic disk