Published March 1979 | Version v1
Journal article

Surface photometry and mass distributions of spiral galaxies

  • 1. Saint Andrews Univ. (UK). Observatory

Description

A computerized system for performing surface photometry of galaxies is described and illustrated by the results for NGC 157, an isolated SAB(rs)bc galaxy of luminosity class I. An extra outer exponential component has been found in the U, B, V and R reduced profiles. The radial variation of M/L has been studied by extrapolating the observed rotation curve. An explanation for the gross structure and detailed colour and M/L variations has been given in terms of the density wave theory of spiral structure. This explanation implies that the rotation curve NGC 157 is not flat at large radii, approximately 25 kpc, as it would be if a massive halo were present. (author)

Additional details

Additional titles

Subtitle (English)
1. NGC 157

Publishing Information

Journal Title
Mon. Not. R. Astron. Soc.
Journal Volume
186
Journal Issue
3
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
701-715
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
10453616
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Numerical Data
Is Lead record
Yes
Descriptors DEI
COLOR; COSMOLOGICAL MODELS; DATA ACQUISITION SYSTEMS; DATA PROCESSING; DENSITY; EXPERIMENTAL DATA; GALAXIES; GRAPHS; ISOLATED VALUES; LUMINOSITY; MAPS; MASS; PHOTOMETRY; ROTATION; SPATIAL DISTRIBUTION; SPIRAL CONFIGURATION; SURFACES; TELESCOPES
Descriptors DEC
CONFIGURATION; DATA; DATA FORMS; DISTRIBUTION; INFORMATION; MATHEMATICAL MODELS; NUMERICAL DATA; OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES