Local galaxy flows within 5 Mpc

By I. Karachentsev, Dmitry I. Makarov, M. Sharina, A. Dolphin, E. Grebel, D. Geisler, P. Guhathakurta, P. Hodge, V. Karachentseva, A. Sarajedini and 1 more. 2002

141 citations recorded by the source corpus.

We present Hubble Space Telescope/WFPC2 images of sixteen dwarf galaxies as part of our snapshot survey of nearby galaxy candidates. We derive their distances from the luminosity of the tip of the red giant branch stars with a typical

Subfields: Astronomy and Astrophysics, Electrical and Electronic Engineering, Instrumentation

View Paper: https://www.semanticscholar.org/paper/a708f5ccf816f1ee542a2a29cb688d288fc114b3

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Citations in the corpus

Star Formation Properties of a Large Sample of Irregular Galaxies (2004, unknown): “…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) Maiz-Apellaniz, Cieza, & Mackenty 2002; (20) Makarova et al. 1998; (21)…”
The Baryonic Tully-Fisher Relation of Galaxies with Extended Rotation Curves and the Stellar Mass of Rotating Galaxies (2005, background): “The relative distance uncertainty for NGC 2915 is also uncomfortably large (Meurer, Mackie, & Carignan 1994; Karachentsev et al. 2003).”
Our Peculiar Motion Away from the Local Void (2007, result): “This motion differs from zero with only marginal significance and is consistent with the observation by Karachentsev et al. (2003) that nearby groups and individual isolated galaxies adhere to the local expansion with a dispersion of only 40 km s−1.”
Advanced Camera for Surveys Imaging of 25 Galaxies in Nearby Groups and in the Field (2005, methodology): “The derived TRGB distance to NGC 247, 3.65 Mpc, agrees with the distance estimate, 4.1 Mpc, obtained from the TF relation (Karachentsev et al. 2003b).”
Distances to nearby galaxies in Sculptor (2003, background): “As was noted by Jerjen et al.(1998) and Karachentsev et al.(2003), the galaxy complexes in Sculptor and Canes Venatici together with the Local Group form an amorphous filament extending over ∼10 Mpc.”
The Local Group and Other Neighboring Galaxy Groups (2005, methodology): “For the sample of 34 members of the cloud, Karachentsev et al. (2003a) derived the radial velocity dispersion 50 km s −1 , the mean linear projected radius 760 kpc, and the mass estimates: 360 × 10 10 M ⊙ (vir) and 190 × 10 10 M ⊙ (orb).”
The search for failed supernovae with the Large Binocular Telescope: first candidates (2014, unknown): “References – (1) Gerke et al. 2011; (2) Jacobs et al. 2009; (3) Shappee & Stanek 2011; (4) Herrmann et al. 2008; (5) Karachentsev et al. 2004; (6) Karachentsev et al. 2003; (7) Willick et al. 1997; (8) Drozdovsky & Karachentsev 2000; (9) Verdes-Montenegro et al. 2000; (10) Theureau et al. 2007;…”
THE GHOSTS SURVEY. I. HUBBLE SPACE TELESCOPE ADVANCED CAMERA FOR SURVEYS DATA (2011, methodology): “As the likelihood of observing disk galaxies at such high inclinations is low, they are typically observed at distances greater than the limits of the Karachentsev et al. (2003c) catalog and so require longer exposures.”
Associations of Dwarf Galaxies (2006, background): “Now that excellent TRGB distances are becoming available, it is becoming evident that this structure breaks up into distinct foreground and background components that are completely confused in velocity – 14 – and position on the sky (Karachentsev et al. 2003b).”
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. ”
A Catalog of Neighboring Galaxies (2004, background): “+67 54 49 Karachentsev et al. 2003b; ph: Bremnes et al. 1998 09 50 10.0...........”