ar X iv : a st ro - p h / 04 01 55 8 v 1 2 6 Ja n 20 04 Cepheids and Long Period Variables in NGC 4395
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چکیده
Repeated imaging observations of NGC 4395 were made with the WIYN 3.5 m and the KPNO 2.1 m telescopes. From the photometry of the resolved brighter stars in this galaxy eleven Cepheids with periods ranging between 12 and 90 days have been identified. The true distance modulus has been derived from the apparent distance moduli in g, r and i.
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تاریخ انتشار 2004