The Nature of the X-Ray Binaries in the Whirlpool Galaxy/M51

Date

2018-05

Authors

Bichon, Luis, III

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Abstract

This research consists of the analysis of data from space based observatories such as the Hubble Space Telescope and Chandra X-ray Observatory. The method includes the stellar identification of optical sources in Messier 51 (the Whirlpool Galaxy) found in images from the Hubble Space Telescope. A multi-wavelength analysis (including aperture photometry) is performed on the identified stars, followed by age-dating, and mass estimation. These results are then cross-correlated with the results from preexisting catalogues of X-ray sources. These findings yield a deeper understanding of the nature of the X-ray binaries in the Whirlpool Galaxy and provide greater insight on the X-ray binary formation, and evolution in the galaxy. This knowledge can be generalized to other spiral galaxies much like our own Milky Way.

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Keywords

physics, astrophysics, space, astronomy, stellar, evolution, galaxy, x-ray, Honors College

Citation

Bichon, L. (2018). The nature of the x-ray binaries in the Whirlpool Galaxy/M51 (Unpublished thesis). Texas State University, San Marcos, Texas.

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