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: We request a 190 ks Chandra ACIS-I observation of the spiral galaxy M96 to study the role of dynamics at local and global (galaxy) scales in X-ray binary (XRB) formation and evolution. We will determine if there is an enhancement in the XRB population on local scales per stellar mass and star formation rate. We will leverage the exquisite HST archival multi-band coverage of M96 to assess whether XRB populations are dynamically scattered beyond the stellar population distributions. In combination with recently updated population synthesis modeling, we will use multiwavelength data to discern the nature of any enhancements/scattering in the XRB population and study the age of stellar populations surrounding X-ray binaries and identify counterparts. |
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