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Deep Hubble Space Telescope Imaging of Sextans A. II. Cepheids and Distance

Citation

Dolphin, AE and Saha, A and Skillman, ED and Dohm-Palmer, RC and Tolstoy, E and Cole, AA and Gallagher, JS and Hoessel, JG and Mateo, M, Deep Hubble Space Telescope Imaging of Sextans A. II. Cepheids and Distance, The Astronomical Journal, 125, (3) pp. 1261-1290 . ISSN 0004-6256 (2003) [Refereed Article]

DOI: doi:10.1086/346279

Abstract

We have identified 82 short-period variable stars in Sextans A from deep Wide Field Planetary Camera 2 observations. All the periodic variables appear to be short-period Cepheids, with periods as small as 0.8 days for fundamental mode Cepheids and 0.5 days for first-overtone Cepheids. These objects have been used, along with measurements of the red giant branch (RGB) tip and red clump, to measure a true distance modulus to Sextans A of μ0 = 25.61 ± 0.07, corresponding to a distance of d = 1.32 ±0.04 Mpc. Comparing distances calculated by these techniques, we find that short-period Cepheids (P < 2 days) are accurate distance indicators for objects at or below the metallicity of the Small Magellanic Cloud. As these objects are quite numerous in low-metallicity star-forming galaxies, they have the potential for providing extremely precise distances throughout the Local Group. We have also compared the relative distances produced by other distance indicators. We conclude that calibrations of RR Lyrae stars, the RGB tip, and the red clump are self-consistent, but that there appears to be a small dependence of long-period Cepheid distances on metallicity. Finally, we present relative distances of Sextans A, Leo A, IC 1613, and the Magellanic Clouds.

Item Details

Item Type:Refereed Article
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Galactic Astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:Cole, AA (Dr Andrew Cole)
ID Code:45313
Year Published:2003
Web of Science® Times Cited:49
Deposited By:Physics
Deposited On:2007-07-10
Last Modified:2011-11-28
Downloads:0

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