The central region of NGC 1510

Details The central region of NGC 1510 The central region of NGC 1510

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...132..342e&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 132, no. 2, March 1984, p. 342-350.

Mathematics

Logic

17

A Stars, Elliptical Galaxies, Galactic Nuclei, Stellar Evolution, Stellar Mass Accretion, Wolf-Rayet Stars, H Ii Regions, Halos, Hydrogen, Morphological Indexes, Stellar Color, Stellar Spectra, Stellar Spectrophotometry

Scientific paper

New short-exposure good resolution B, V, and R plates of the central region of NGC 1510 reveal a rather complex central structure of several condensations having different colours. Blue and red IDS spectra of two of these condensations show that they are low-density, slightly metal-poor H II regions with a strong underlying A-star component. One of these condensations contains a small WR star population. Using these new observations, the authors discuss the nature of NGC 1510.

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