Globular clusters in low mass galaxies

Margarita E. Sharina, T. H. Puzia, V. L. Afanasiev, D. I. Makarov, A. E. Dolphin, G. M. Karataeva

Research output

Abstract

We study properties of globular cluster candidates (GCCs) and the diffuse stellar populations in nearby low surface brightness dwarf galaxies, using HST WFPC2 photometry in the V and I bands. Our sample consists of 18 dwarf spheroidal (dSph), 36 dwarf irregular (dIrr), and 3 transition-type galaxies, with projected linear diameters less than 3.5 kpc and mean blue surface brightness >23 mag/arcsec2 situated at the distance 2-6 Mpc in the field and in nearby groups. Our sample dwarf spheroidal galaxies were not detected in HI and are located at the distances of up to ˜1 Mpc away from a nearby bright galaxy. Transition-type galaxies, which are distributed like dSph galaxies, form a very rare class of galaxies. dIrr galaxies show a weaker concentration to the nearest massive neighbors than dSph and transition-type galaxies. At a given surface brightness and luminosity, they exhibit lower mean metallicities than dSphs. In contrast to dIrr galaxies, the majority of dSph galaxies at a similar mean surface brightness
Original languageEnglish
PublisherCambridge University Press
DOIs
Publication statusPublished - 2005

Fingerprint Dive into the research topics of 'Globular clusters in low mass galaxies'. Together they form a unique fingerprint.

Cite this