Andromeda XVII: A new low-luminosity satellite of M31

M. J. Irwin*, A. M. N. Ferguson, A. P. Huxor, N. R. Tanvir, R. A. Ibata, G. F. Lewis

*Awdur cyfatebol y gwaith hwn

    Allbwn ymchwil: Cyfraniad at gyfnodolynErthygladolygiad gan gymheiriaid

    71 Wedi eu Llwytho i Lawr (Pure)

    Crynodeb

    We report the discovery of a new dwarf spheroidal galaxy near M31 on the basis of INT/WFC imaging. The system, Andromeda XVII (And XVII), is located at a projected radius of approximate to 44 kpc from M31, has a line-of-sight distance of 794 +/- 40 kpc measured using the tip of the red giant branch, and therefore lies well within the halo of M31. The color of the red giant branch implies a metallicity of [Fe/H] approximate to -1.9, and we find an absolute magnitude of M-V approximate to -8.5. Three globular clusters lie near the main body of And XVII, suggesting a possible association; if any of these are confirmed, it would make And XVII exceptionally unusual among the faint dSph population. The projected position on the sky of And XVII strengthens an intriguing alignment apparent in the satellite system of M31, although with a caveat about biases stemming from the current area surveyed to significant depth.

    Iaith wreiddiolSaesneg
    Tudalennau (o-i)L17-L20
    Nifer y tudalennau4
    CyfnodolynAstrophysical Journal Letters
    Cyfrol676
    Rhif cyhoeddi1
    Dynodwyr Gwrthrych Digidol (DOIs)
    StatwsCyhoeddwyd - 20 Maw 2008

    Ôl bys

    Gweld gwybodaeth am bynciau ymchwil 'Andromeda XVII: A new low-luminosity satellite of M31'. Gyda’i gilydd, maen nhw’n ffurfio ôl bys unigryw.

    Dyfynnu hyn