Surface photometry of edge-on galaxies. VI - NGC 4452 and NGC 4762

Details Surface photometry of edge-on galaxies. VI - NGC 4452 and NGC 4762 Surface photometry of edge-on galaxies. VI - NGC 4452 and NGC 4762

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339..783h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 15, 1989, p. 783-802.

Other

17

Astronomical Photometry, Barred Galaxies, Galactic Structure, Lenticular Bodies, Astronomical Photography, Brightness Distribution, Galactic Bulge, Optical Thickness

Scientific paper

It is shown that the lenses of NGC 4452 and NGC 4762 are less steep in the vertical luminosity profile than the isothermal disk model. The presence of humps in the major axis profiles suggests that NGC 4452 and NGC 4762 as well NGC 1381 are edge-on barred lenticular galaxies. It is believed that more observations of edge-on lenticular galaxies with high spatial resolutions are required to clarify the nature of extremely thin components.

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