C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: The unique high resolution capabilities of Chandra HETG gratings will allow to study in depth the stellar wind properties of the early B supergiant V662 Cas, the mass donor of the wind accreting pulsar 4U0114+65. The goal is to put observational constraints on the current models of stellar winds in massive stars using the point like source of ionizing X-rays as a probe. Together with existing observations, we will study the stellar wind clumping across the spectral sequence. In particular, we want to study the wind clumping of V662 Cas, the coolest (B1I) among the massive donors in any HMXB, and answer fundamental questions: is the wind clumped or smooth at r = 1.5R*? What is the role of the bistability jump in the formation/destruction of clumps? |
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