Photometric deprojection of edge-on galaxies
- 1 April 2000
- journal article
- Published by Pleiades Publishing Ltd in Astronomy Letters
- Vol. 26 (4) , 219-224
- https://doi.org/10.1134/1.20385
Abstract
Photometric deprojection is used to determine the stellar-disk and bulge parameters for several edge-on galaxies from the FGC catalog. The assumption that the galaxies of our sample belonging to the fourth (i.e., lowest) surface-brightness class in the FGC are edge-on, low-surface-brightness (LSB) galaxies is considered.Keywords
All Related Versions
This publication has 10 references indexed in Scilit:
- The Ursa Major Cluster of Galaxies. II. Bimodality of the Distribution of Central Surface BrightnessesThe Astrophysical Journal, 1997
- Low-Surface-Brightness Galaxies: Hidden Galaxies RevealedPublications of the Astronomical Society of the Pacific, 1997
- Does Low Surface Brightness Mean Low Density?The Astrophysical Journal, 1996
- Tidally-triggered disk thickening. I. ObservationsAstronomy and Astrophysics Supplement Series, 1996
- The number, luminosity and mass density of spiral galaxies as a function of surface brightnessMonthly Notices of the Royal Astronomical Society, 1996
- Multi‐colour surface photometry of a sample of HI‐detected late type galaxiesAstronomische Nachrichten, 1996
- Properties of the class of giant low surface brightness spiral galaxiesThe Astronomical Journal, 1995
- Structural characteristics and stellar composition of low surface brightness disk galaxiesThe Astronomical Journal, 1994
- Flat Galaxy CatalogueAstronomische Nachrichten, 1993
- Flat edge-on galaxies. Atlas and photometryAstronomical & Astrophysical Transactions, 1992