The M 81 group of galaxies: New distances, kinematics and structure ?;??

By I. Karachentsev, A. Dolphin, D. Geisler, E. Grebel, P. Guhathakurta, P. Hodge, V. Karachentseva, A. Sarajedini, Patrick Seitzer, M. Sharina. 2002

209 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/716328baae1170faad9d3c8a421d90036275f257

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Citations in the corpus

A Nearby Repeating Fast Radio Burst in the Direction of M81 (2021, background): “We then describe our search for a host and propose that M81, a nearby early-type grand-design spiral galaxy at 3.63± 0.34Mpc (Freedman et al. 1994; Karachentsev et al. 2002), is the most likely FRB host.”
Investigations of dust heating in M81, M83 and NGC 2403 with the Herschel Space Observatory (2011, background): “M81 (NGC 3031) is an Sab galaxy (de Vaucouleurs et al. 1991) that is the brightest galaxy in the M81 Group (Karachentsev et al. 2002).”
Local galaxy flows within 5 Mpc (2002, background): “…group, (4) mean projected linear radius of the group, (5) radial velocity dispersion, (6) absolute B magnitude of the brightest member, (7) integrated luminosity of the group, (8,9) virial and orbital (Karachentsev et al. 2002a) mass estimate normalized to the luminosity unit, (10) crossing time.”
The Local Group and Other Neighboring Galaxy Groups (2005, background): “…on nearby galaxy distances and radial velocities allowed us to determine virial and total masses of four of the nearest complexes: Milky Way+M31 (Karachentsev et al. 2002c), M81+NGC2403 (Karachentsev et al. 2002a), CenA+M83 (Karachentsev et al. 2002b), and IC342+Maffei (Karachentsev et al.…”
Galaxy Groups Within 3500 km s−1 (2017, methodology): “Subsequent imaging with the Hubble Space Telescope has provided distance estimates for about 400 nearby galaxies from the apparent magnitude of the tip of the red giant branch in each system (Karachentsev et al. 2002, 2006; Jacobs et al. 2009).”
An Hα Imaging Survey of Galaxies in the Local 11 Mpc Volume (2004, unknown): “—(1) Cote et al. 1997: Cen A group; (2) Ferrerese et al. 2000; (3) Ferrerese et al. 2000: N1023 group (N925 ceph); (4) Fingerhut et al. 2007; (5) Freedman et al. 2001; (6) Irwin et al. 2007; (7) Karachentsev et al. 2006; (8) Karachentsev et al. 2007; (9) KKH04: Cen A group; (10) KKH04: Crone et al. ”
CONFIRMATION OF FAINT DWARF GALAXIES IN THE M81 GROUP (2013, methodology): “Attempts to measure the distances using the TRGB found distances that more likely applied to the major galaxies themselves (Karachentsev et al. 2002).”
Associations of Dwarf Galaxies (2006, background): “It is a factor two more distant than the zero velocity surface separating Local Group infall from cosmic expansion (Karachentsev et al. 2002a) but still within the zero energy surface (Peirani & Pacheco 2005) so conceivably is bound to the Local Group.”
The Hubble Flow around the Centaurus A/M83 Galaxy Complex (2006, background): “Karachentsev et al. (2002a, 2002b, 2003) have shown that the M81/NGC 2403, Cen A/M83, and Maffei 1/ IC 342 groups are all ‘‘dumbbell’’ systems like the Local Group (LG).”
Star Formation Properties of a Large Sample of Irregular Galaxies (2004, unknown): “…Maŕin-Franch, & Aparicio 2003; (11) Hunter 2001; (12) Karachentsev, Aparicio, & Makarova 1999; (13) Karachentsev, Musella, & Grimaldi 1996; (14) Karachentsev et al. 2002; (15) Karachentsev et al. 2003a; (16) Karachentsev et al. 2003b; (17) Lee et al. 1999; (18) Lee & Kim 2000; (19)…”