NGC 615
Apparent magnitude (V) | 11.5 |
---|---|
Characteristics | |
Type | SA(rs)b [1] |
Apparent size (V) | 3.6′ × 1.4′[1] |
Other designations | |
MCG -01-05-008, PGC 5897[1] |
NGC 615 is an unbarred
The galaxy is included in the Herschel 400 Catalogue. It lies about three degrees northeast from Theta Ceti.[4]
Characteristics
The galaxy has been found to possess a chemically and dynamically decoupled nucleus.[5] Further observations revealed two decoupled components, with the outer one identified as a disk. In the centre of the galaxy (<3" / 0.3 kpc) was found to exist an inclined circumnuclear disk. The stars in the circumnuclear disk have solar metallicity and their median age was determined at 5 billion years. In the bulge of NGC 615 (3"-6") was detected a counterrotating gaseous component.[5]
Further away of the centre (8-30") lies the inner decoupled component, where
The outer disk demonstrates a pair of low-contrast outer spiral arms or, more likely, a ring. Its inclination with respect to the line of sight is no more than 60°.[5]
References
- ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 615. Retrieved 2016-01-18.
- ^ Seligman, Courtney. "NGC 615 (= PGC 5897)". Celestial Atlas. Retrieved 19 November 2018.
- S2CID 119194025.
- ISBN 978-0521858939.
- ^ doi:10.1086/320368.
- S2CID 39130734.
External links
- NGC 615 on