Published September 15, 1988 | Version v1
Journal article

NGC 6776 'The Pentagon' - an old merger?

  • 1. Leicester Univ. (UK). Dept. of Physics
  • 2. California Inst. of Tech., Pasadena (USA)
  • 3. Observatoire de Paris, Section de Meudon, 92 (France)

Description

Photometric and spectroscopic observations of NGC 6776 are presented. Photographic and CCD images show that this galaxy has perturbed and chaotic outer isophotes and possesses at least one tidal tail. Spectroscopic observations show that the system is rapidly rotating, with low stellar velocity dispersion, atypical of early-type systems. These characteristics strongly suggest that this galaxy has undergone a merger with a second system. However, the colour distribution shows no evidence for the presence of young stars, while IRAS data indicate that the system is relatively free of dust. We conclude that this galaxy is the remnant of a merger occurring at least 109yr ago, making it the oldest merger known, and involving at least one dust-poor disc system. (author)

Additional details

Publishing Information

Journal Title
Monthly Notices of the Royal Astronomical Society
Journal Volume
234
Journal Issue
2
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
247-268
ISSN
0035-8711
CODEN
MNRAA

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
20004771
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Numerical Data
Descriptors DEI
BRIGHTNESS; COALESCENCE; COLOR; DISTURBANCES; EXPERIMENTAL DATA; GALAXIES; IMAGES; MAPS; PHOTOMETRY; ROTATION; SPATIAL DISTRIBUTION; SPECTROSCOPY; VISIBLE RADIATION
Descriptors DEC
DATA; DISTRIBUTION; ELECTROMAGNETIC RADIATION; INFORMATION; NUMERICAL DATA; OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS