New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683

Author:

Crosby Ethan1,Jerjen Helmut1,Müller Oliver2,Pawlowski Marcel3,Mateo Mario4,Dirnberger Markus1

Affiliation:

1. Research School of Astronomy and Astrophysics, Australian National University , Canberra, ACT 2611 , Australia

2. Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Féd’erale de Lausanne (EPFL) , CH-1290 Sauverny , Switzerland

3. Leibniz-Institut für Astrophysik Potsdam , An der Sternwarte 16, D-14482 Potsdam , Germany

4. Department of Astronomy, University of Michigan , 1085 S. University Ave., Ann Arbor, MI 48109 , USA

Abstract

ABSTRACT We present initial results of a survey of host L* galaxies environments in the Local Volume ($D\lt 10\,$ Mpc) searching for satellite dwarf galaxy candidates using the wide-field Hyper Suprime-Cam imager on the 8 m Subaru Telescope. This paper presents complete results on NGC2683 ($M_{B_T,0}=-19.62$, $D=9.36\, \mathrm{ Mpc}$, $v_{\odot }=411\, \mathrm{ km\, s}^{-1}$), an isolated Sc spiral galaxy in the Leo Spur. At the distance of NGC2683, we image the complete volume out to projected radii of $380\, \mathrm{ kpc}$ using a hexagonal arrangement of 7 pointings. Direct inspection of the images is complete down to Mg ∼ −11 and has revealed four new satellite galaxy candidates, two of which have been independently discovered by other researchers. Assuming the distance of NGC2683, these candidates span luminosities −12 < Mg < −9 and effective radii 150 pc <re < 1100 pc and are found to be morphologically reminiscent of satellite galaxies in the Local Group. These four new candidates add to the eight already known. A principle component analysis of the 2D projected distribution of the 12 satellite galaxies of NGC2683 reveals a flattened projected disc of satellites, with axis ratio b/a = 0.23. This flattening in the 2D projected system of satellites is a 1 per cent outlier of simulated isotropic satellite systems but is mostly consistent with satellite distributions of comparable galaxy environments in the IllustrisTNG simulation. This indicates the possible presence of a satellite plane, which will need to be investigated with follow-up observations.

Funder

Australian Research Council

Swiss National Science Foundation

Leibniz

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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