Kavli Affiliate: Deepto Chakrabarty | First 5 Authors: Pragati Pradhan, Carlo Ferrigno, Biswajit Paul, Enrico Bozzo, Ileyk El Mellah | Summary: Winds of massive stars are suspected to be inhomogeneous (or clumpy), which biases the measures of their mass loss rates. In High Mass X-ray Binaries (HMXBs), the compact object can be used as an […]
Continue.. Clumpy wind studies and the non-detection of cyclotron line in OAO 1657-415