A new milky way dwarf satellite in canes venatici

D. B. Zucker, V. Belokurov, N. W. Evans, M. I. Wilkinson, M. J. Irwin, T. Sivarani, S. Hodgkin, D. M. Bramich, J. M. Irwin, G. Gilmore, B. Willman, S. Vidrih, M. Fellhauer, P. C. Hewett, T. C. Beers, E. F. Bell, E. K. Grebel, D. P. Schneider, H. J. Newberg, R. F G Wyse & 13 others C. M. Rockosi, B. Yanny, R. Lupton, J. A. Smith, J. C. Barentine, H. Brewington, J. Brinkmann, M. Harvanek, S. J. Kleinman, J. Krzesinski, D. Long, A. Nitta, S. A. Snedden

Research output: Contribution to journalArticle

274 Citations (Scopus)

Abstract

In this Letter, we announce the discovery of a new dwarf satellite of the Milky Way, located in the constellation Canes Venatici. It was found as a stellar overdensity in the north Galactic cap using Sloan Digital Sky Survey Data Release 5 (SDSS DR5). The satellite's color-magnitude diagram shows a well-defined red giant branch as well as a horizontal branch. As judged from the tip of the red giant branch, it lies at a distance of ∼220 kpc. Based on the SDSS data, we estimate an absolute magnitude of Mv ∼ -7.9, a central surface brightness of μ0,v ∼ 28 mag arcsec -2, and a half-light radius of ∼8′.!5 (∼550 pc at the measured distance). The outer regions of Canes Venatici appear extended and distorted. The discovery of such a faint galaxy in proximity to the Milky Way strongly suggests that more such objects remain to be found.

Original languageEnglish
JournalAstrophysical Journal
Volume643
Issue number2 II
DOIs
Publication statusPublished - 1 Jun 2006
Externally publishedYes

Fingerprint

constellations
color-magnitude diagram
caps
proximity
brightness
diagram
galaxies
radii
estimates

Keywords

  • Galaxies: dwarf
  • Galaxies: individual (Canes Venatici)
  • Local Group

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Zucker, D. B., Belokurov, V., Evans, N. W., Wilkinson, M. I., Irwin, M. J., Sivarani, T., ... Snedden, S. A. (2006). A new milky way dwarf satellite in canes venatici. Astrophysical Journal, 643(2 II). https://doi.org/10.1086/505216

A new milky way dwarf satellite in canes venatici. / Zucker, D. B.; Belokurov, V.; Evans, N. W.; Wilkinson, M. I.; Irwin, M. J.; Sivarani, T.; Hodgkin, S.; Bramich, D. M.; Irwin, J. M.; Gilmore, G.; Willman, B.; Vidrih, S.; Fellhauer, M.; Hewett, P. C.; Beers, T. C.; Bell, E. F.; Grebel, E. K.; Schneider, D. P.; Newberg, H. J.; Wyse, R. F G; Rockosi, C. M.; Yanny, B.; Lupton, R.; Smith, J. A.; Barentine, J. C.; Brewington, H.; Brinkmann, J.; Harvanek, M.; Kleinman, S. J.; Krzesinski, J.; Long, D.; Nitta, A.; Snedden, S. A.

In: Astrophysical Journal, Vol. 643, No. 2 II, 01.06.2006.

Research output: Contribution to journalArticle

Zucker, DB, Belokurov, V, Evans, NW, Wilkinson, MI, Irwin, MJ, Sivarani, T, Hodgkin, S, Bramich, DM, Irwin, JM, Gilmore, G, Willman, B, Vidrih, S, Fellhauer, M, Hewett, PC, Beers, TC, Bell, EF, Grebel, EK, Schneider, DP, Newberg, HJ, Wyse, RFG, Rockosi, CM, Yanny, B, Lupton, R, Smith, JA, Barentine, JC, Brewington, H, Brinkmann, J, Harvanek, M, Kleinman, SJ, Krzesinski, J, Long, D, Nitta, A & Snedden, SA 2006, 'A new milky way dwarf satellite in canes venatici', Astrophysical Journal, vol. 643, no. 2 II. https://doi.org/10.1086/505216
Zucker DB, Belokurov V, Evans NW, Wilkinson MI, Irwin MJ, Sivarani T et al. A new milky way dwarf satellite in canes venatici. Astrophysical Journal. 2006 Jun 1;643(2 II). https://doi.org/10.1086/505216
Zucker, D. B. ; Belokurov, V. ; Evans, N. W. ; Wilkinson, M. I. ; Irwin, M. J. ; Sivarani, T. ; Hodgkin, S. ; Bramich, D. M. ; Irwin, J. M. ; Gilmore, G. ; Willman, B. ; Vidrih, S. ; Fellhauer, M. ; Hewett, P. C. ; Beers, T. C. ; Bell, E. F. ; Grebel, E. K. ; Schneider, D. P. ; Newberg, H. J. ; Wyse, R. F G ; Rockosi, C. M. ; Yanny, B. ; Lupton, R. ; Smith, J. A. ; Barentine, J. C. ; Brewington, H. ; Brinkmann, J. ; Harvanek, M. ; Kleinman, S. J. ; Krzesinski, J. ; Long, D. ; Nitta, A. ; Snedden, S. A. / A new milky way dwarf satellite in canes venatici. In: Astrophysical Journal. 2006 ; Vol. 643, No. 2 II.
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AU - Zucker, D. B.

AU - Belokurov, V.

AU - Evans, N. W.

AU - Wilkinson, M. I.

AU - Irwin, M. J.

AU - Sivarani, T.

AU - Hodgkin, S.

AU - Bramich, D. M.

AU - Irwin, J. M.

AU - Gilmore, G.

AU - Willman, B.

AU - Vidrih, S.

AU - Fellhauer, M.

AU - Hewett, P. C.

AU - Beers, T. C.

AU - Bell, E. F.

AU - Grebel, E. K.

AU - Schneider, D. P.

AU - Newberg, H. J.

AU - Wyse, R. F G

AU - Rockosi, C. M.

AU - Yanny, B.

AU - Lupton, R.

AU - Smith, J. A.

AU - Barentine, J. C.

AU - Brewington, H.

AU - Brinkmann, J.

AU - Harvanek, M.

AU - Kleinman, S. J.

AU - Krzesinski, J.

AU - Long, D.

AU - Nitta, A.

AU - Snedden, S. A.

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N2 - In this Letter, we announce the discovery of a new dwarf satellite of the Milky Way, located in the constellation Canes Venatici. It was found as a stellar overdensity in the north Galactic cap using Sloan Digital Sky Survey Data Release 5 (SDSS DR5). The satellite's color-magnitude diagram shows a well-defined red giant branch as well as a horizontal branch. As judged from the tip of the red giant branch, it lies at a distance of ∼220 kpc. Based on the SDSS data, we estimate an absolute magnitude of Mv ∼ -7.9, a central surface brightness of μ0,v ∼ 28 mag arcsec -2, and a half-light radius of ∼8′.!5 (∼550 pc at the measured distance). The outer regions of Canes Venatici appear extended and distorted. The discovery of such a faint galaxy in proximity to the Milky Way strongly suggests that more such objects remain to be found.

AB - In this Letter, we announce the discovery of a new dwarf satellite of the Milky Way, located in the constellation Canes Venatici. It was found as a stellar overdensity in the north Galactic cap using Sloan Digital Sky Survey Data Release 5 (SDSS DR5). The satellite's color-magnitude diagram shows a well-defined red giant branch as well as a horizontal branch. As judged from the tip of the red giant branch, it lies at a distance of ∼220 kpc. Based on the SDSS data, we estimate an absolute magnitude of Mv ∼ -7.9, a central surface brightness of μ0,v ∼ 28 mag arcsec -2, and a half-light radius of ∼8′.!5 (∼550 pc at the measured distance). The outer regions of Canes Venatici appear extended and distorted. The discovery of such a faint galaxy in proximity to the Milky Way strongly suggests that more such objects remain to be found.

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KW - Galaxies: individual (Canes Venatici)

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