NGC 6776 'The Pentagon' - an old merger?
Creators
- 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