Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-30871
Belokurov, V; Walker, M G; Evans, N W; Gilmore, G; Irwin, M J; Mateo, M; Mayer, L; Olszewski, E; Bechtold, J; Pickering, T (2009). The discovery of Segue 2: a prototype of the population of satellites of satellites. Monthly Notices of the Royal Astronomical Society, 397(4):1748-1755.
View at publisher
We announce the discovery of a new Milky Way satellite Segue 2 found in the data of the Sloan Extension for Galactic Understanding and Exploration (SEGUE). We followed this up with deeper imaging and spectroscopy on the Multiple Mirror Telescope (MMT). From this, we derive a luminosity of Mv=−2.5 , a half-light radius of 34 pc and a systemic velocity of ∼−40 km s−1 . Our data also provide evidence for a stream around Segue 2 at a similar heliocentric velocity, and the SEGUE data show that it is also present in neighbouring fields. We resolve the velocity dispersion of Segue 2 as 3.4 km s−1 and the possible stream as ∼7 km s−1 . This object shows points of comparison with other recent discoveries, Segue 1, Boo II and Coma. We speculate that all four objects may be representatives of a population of satellites of satellites – survivors of accretion events that destroyed their larger but less dense parents. They are likely to have formed at redshifts z > 10 and are good candidates for fossils of the reionization epoch.
25 downloads since deposited on 25 Feb 2010
10 downloads since 12 months
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Dewey Decimal Classification:||530 Physics|
|Uncontrolled Keywords:||galaxies: dwarf; galaxies: individual: Segue 2; Local Group|
|Deposited On:||25 Feb 2010 19:49|
|Last Modified:||27 Nov 2013 23:12|
|Funders:||Alfred P. Sloan Foundation|
|Additional Information:||The attached file is a preprint (accepted version) of an article published in Monthly Notices of the Royal Astronomical Society. The definitive version is available at www3.interscience.wiley.com|
Users (please log in): suggest update or correction for this item
Repository Staff Only: item control page