Distance of M83 and of the Centaurus group

Journal Article · Sat Sep 01 04:00:00 EDT 1979 · Astron. J.; (United States)

DOI:https://doi.org/10.1086/112539· OSTI ID:6093780

de Vaucouleurs, G

The distances of eight probable or possible bright (B/sup 0//sub T/<11) members of the Centaurus group of galaxies are derived from several secondary and tertiary indicators and from redshifts. Except for the heavily obscured Circinus galaxy, the different methods are in good systematic agreement. The best-determined distance is that of M83 with ..mu../sub 0/=27.84 +- 0.15 (m.e.) and ..delta..=3.70 +- 0.25 Mpc from six indicators. The group, centered at supergalactic coordinates L=154/sup 0/, B=-2/sup 0/, is at a mean distance <..delta..> =3.3 +- 0.4 Mpc; it covers an elongated area 33/sup 0/ x 18/sup 0/=1.8 x 1.0 Mpc, parallel to the supergalactic plane, and has a depth of approximately 2 Mpc (2.0< or =..delta..< or =4.0 Mpc) in the line of sight. Eight dwarf galaxies recently discussed by Webster et al. are confirmed to be members or probable members of the group. The Fourcade--Figueroa galaxy (A1332-45) is probably a background object at ..delta..approx. =5.3 Mpc; the Circinus galaxy (A1409-65) is probably a field galaxy at ..delta..approx. =4 Mpc, but additional members between it and the group may be hidden near the galactic plane. The velocity dispersion, sigma/sub v/approx. =70 km s/sup -1/, may be interpreted either as evidence for stability (bound group) or instability (expanding association or accidental grouping). The presence of three early-type systems (NGC 5102, 5128, 5253) in a group dominated by late-type spirals (NGC 4945, 5068, 5236) and magellanic irregulars is unusual and suggestive of a chance encounter.

• Research Organization: Department of Astronomy and McDonald Observatory, The University of Texas, Austin, Texas 78712
• OSTI ID: 6093780
• Journal Information: Astron. J.; (United States), Journal Name: Astron. J.; (United States) Vol. 84:9; ISSN ANJOA
• Country of Publication: United States
• Language: English

Related Subjects

640105* -- Astrophysics &amp; Cosmology-- Galaxies
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC RADIO SOURCES
DISTANCE
ERUPTIVE VARIABLE STARS
GALAXIES
GALAXY CLUSTERS
H2 REGIONS
LUMINOSITY
MORPHOLOGY
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
RADIO GALAXIES
RED SHIFT
STARS
SUPERNOVAE
VARIABLE STARS