A new giant stellar structure in the outer halo of M31

作者：Zucker DB^*; Kniazev AY; Bell EF; Martinez Delgado D; Grebel EK; Rix HW; Rockosi CM; Holtzman JA; Walterbos RAM; Ivezic E; Brinkmann J; Brewington H; Harvanek M; Kleinman SJ; Krzesinski J; Lamb DQ; Long D; Newman PR; Nitta A; Snedden SA

来源：Astrophysical Journal, 2004, 612(2): L117-L120.

DOI：10.1086/424706

• galaxies : dwarf
• galaxies : evolution
• galaxies : general
• galaxies : individual (M31)
• galaxies : stellar content
• Local Group

The Sloan Digital Sky Survey has revealed an overdensity of luminous red giant stars similar to3degrees ( 40 projected kpc) to the northeast of M31, which we have called Andromeda NE. The line-of-sight distance to Andromeda NE is within similar to50 kpc of M31; Andromeda NE is not a physically unrelated projection. Andromeda NE has a g-band absolute magnitude of similar to-11.6 and a central surface brightness of similar to29 mag arcsec(-2), making it nearly 2 orders of magnitude more diffuse than any known Local Group dwarf galaxy at that luminosity. Based on its distance and morphology, Andromeda NE is likely undergoing tidal disruption. Andromeda NE's red giant branch color is unlike that of M31' s present-day outer disk or the stellar stream reported by Ibata et al., arguing against a direct link between Andromeda NE and these structures. However, Andromeda NE has a red giant branch color similar to that of the G1 clump; it is possible that these structures are both material torn off of M31' s disk in the distant past or that these are both part of one ancient stellar stream.

• 出版日期2004-9-10