The dwarf spheroidal galaxy DDO 44: stellar populations and distance

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dc.creatorKarachentsev, I. D.
dc.creatorSharina, M. E.
dc.creatorGrebel, E. K.
dc.creatorDolphin, A. E.
dc.creatorGeisler, D.
dc.creatorGuhathakurta, P.
dc.creatorHodge, P. W.
dc.creatorKarachentseva, V. E.
dc.creatorSarajedini, A.
dc.creatorSeitzer, P.
dc.date1999-10-21
dc.date.accessioned2026-07-07T02:33:59Z
dc.date.available2026-07-07T02:33:59Z
dc.descriptionWe present ground-based and HST WFPC2 imaging of the nearby low surface brightness dwarf spheroidal galaxy DDO 44. For the first time DDO 44 was resolved into stars. The resulting color-magnitude diagram for about 1290 stars shows the red giant branch with a tip at I=(23.55+-0.15) mag, which yields a distance of (3.2+-0.2) Mpc consistent with membership of DDO 44 in the NGC 2403 group. The linear separation of DDO 44 from NGC 2403 is 75 kpc on the sky and (30+-450) kpc along the line of sight. The relationship between the dwarf galaxy's absolute R magnitude of -13.1 mag, its central surface brightness of 24.1 mag/square arcsec, and its mean metallicity of -1.7 dex follow the trend for other nearby dwarf spheroidal galaxies. One globular cluster candidate has also been identified in DDO 44.
dc.descriptionAstronomy & Astrophysics Main Journal, accepted. 7 figures (2 jpg images, 5 postscript files)
dc.identifierhttps://arxiv.org/abs/astro-ph/9910402
dc.identifierhttp://arxiv.org/abs/astro-ph/9910402
dc.identifier1999, A&A, 352, 399-405
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15066
dc.subjectAstrophysics
dc.titleThe dwarf spheroidal galaxy DDO 44: stellar populations and distance
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