SIMBAD references

2016MNRAS.457L.103R - Mon. Not. R. Astron. Soc., 457, L103-L107 (2016/March-3)

Satellite accretion in action: a tidally disrupting dwarf spheroidal around the nearby spiral galaxy NGC 253.

ROMANOWSKY A.J., MARTINEZ-DELGADO D., MARTIN N.F., MORALES G., JENNINGS Z.G., GABANY R.J., BRODIE J.P., GREBEL E.K., SCHEDLER J. and SIDONIO M.

Abstract (from CDS):

We report the discovery of NGC 253-dw2, a dwarf spheroidal (dSph) galaxy candidate undergoing tidal disruption around a nearby spiral galaxy, NGC 253 in the Sculptor group: the first such event identified beyond the Local Group. The dwarf was found using small-aperture amateur telescopes, and followed up with Suprime-Cam on the 8 m Subaru Telescope in order to resolve its brightest stars. Using g- and Rc-band photometry, we detect a red giant branch consistent with an old, metal-poor stellar population at a distance of ∼3.5 Mpc. From the distribution of likely member stars, we infer a highly elongated shape with a semimajor axis half-light radius of (2 ± 0.4) kpc. Star counts also yield a luminosity estimate of ∼2 x 106 L☉,V (MV ∼ -10.7). The morphological properties of NGC 253-dw2 mark it as distinct from normal dSphs and imply ongoing disruption at a projected distance of ∼50 kpc from the main galaxy. Our observations support the hierarchical paradigm wherein massive galaxies continuously accrete less massive ones, and provide a new case study for dSph infall and dissolution dynamics. We also note the continued efficacy of small telescopes for making big discoveries.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): galaxies: dwarf - galaxies: individual: NGC 253 - galaxies: interactions

Nomenclature: NAME NGC 253-dw2 N=1.

Simbad objects: 14

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