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Globular clusters in low mass galaxies. / Sharina, Margarita E.; Puzia, T. H.; Afanasiev, V. L.; Makarov, D. I.; Dolphin, A. E.; Karataeva, G. M.

In: Proceedings of the International Astronomical Union, Vol. 1, No. C198, 2005, p. 409-412.

Research output: Contribution to journal › Conference article › peer-review

Harvard

Sharina, ME, Puzia, TH, Afanasiev, VL, Makarov, DI, Dolphin, AE & Karataeva, GM 2005, 'Globular clusters in low mass galaxies', Proceedings of the International Astronomical Union, vol. 1, no. C198, pp. 409-412. https://doi.org/10.1017/S1743921305004199

APA

Sharina, M. E., Puzia, T. H., Afanasiev, V. L., Makarov, D. I., Dolphin, A. E., & Karataeva, G. M. (2005). Globular clusters in low mass galaxies. Proceedings of the International Astronomical Union, 1(C198), 409-412. https://doi.org/10.1017/S1743921305004199

Vancouver

Sharina ME, Puzia TH, Afanasiev VL, Makarov DI, Dolphin AE, Karataeva GM. Globular clusters in low mass galaxies. Proceedings of the International Astronomical Union. 2005;1(C198):409-412. https://doi.org/10.1017/S1743921305004199

Author

Sharina, Margarita E. ; Puzia, T. H. ; Afanasiev, V. L. ; Makarov, D. I. ; Dolphin, A. E. ; Karataeva, G. M. / Globular clusters in low mass galaxies. In: Proceedings of the International Astronomical Union. 2005 ; Vol. 1, No. C198. pp. 409-412.

BibTeX

@article{26553cda6a324bd3a8b902a18784ee10,
title = "Globular clusters in low mass galaxies",
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",
author = "Sharina, {Margarita E.} and Puzia, {T. H.} and Afanasiev, {V. L.} and Makarov, {D. I.} and Dolphin, {A. E.} and Karataeva, {G. M.}",
year = "2005",
doi = "10.1017/S1743921305004199",
language = "English",
volume = "1",
pages = "409--412",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "C198",

}

RIS

TY - JOUR

T1 - Globular clusters in low mass galaxies

AU - Sharina, Margarita E.

AU - Puzia, T. H.

AU - Afanasiev, V. L.

AU - Makarov, D. I.

AU - Dolphin, A. E.

AU - Karataeva, G. M.

PY - 2005

Y1 - 2005

N2 - 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

AB - 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

U2 - 10.1017/S1743921305004199

DO - 10.1017/S1743921305004199

M3 - Conference article

VL - 1

SP - 409

EP - 412

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - C198

ER -

ID: 73930095