Variable Stars in IC 5152

Computer Science

Scientific paper

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Scientific paper

One of the best methods to determine the distance to a (nearby) galaxy is to measure the periods and magnitudes of the so-called cepheids in the galaxy. The cepheids are variable stars and they are found by comparing photographic plates of the galaxy from different nights. Drs. Svend Laustsen and Gustav Tammann from the Scientific Group at ESO/Geneva have just analysed such plates of the IC 5152 galaxy:

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