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| NGC 7603 | |
|---|---|
 | |
| Observation data (J2000.0 epoch) | |
| Constellation | Pisces |
| Right ascension | 23h 18m 56.4s[1] |
| Declination | +00° 14′ 38.2″[1] |
| Redshift | 0.029524±0.000073[1] |
| Heliocentric radial velocity | 8851±22 km/s[1] |
| Galactocentric velocity | 8978±22 km/s[1] |
| Distance | 412.9 ± 28 Mly (126.60 ± 8.58 Mpc)[2] |
| Apparent magnitude (V) | 14.04[1] |
| Characteristics | |
| Type | SA(rs)b: pec Sy1.5[1] |
| Apparent size (V) | 1.5 × 1.0 moa[1] |
| Other designations | |
| NGC 7603, UGC 12493, MCG 0-59-21, MK 530, PGC 71035, IRAS23163-0001, UM 156, ARP 92, ZWG 380.26[3] | |
References: NGC+7603[1] | |
NGC 7603 is a spiral Seyfert galaxy in the constellation Pisces.[1] It is listed (as Arp 92) in the Atlas of Peculiar Galaxies.[4] It is interacting with the smaller elliptical galaxy PGC 71041 nearby.[1]
This galaxy pair has long been a cornerstone for those who are critical of the view that the universe is expanding, and advocates for non-standard cosmology such as Halton Arp, Fred Hoyle, and others.[like whom?][5][6] This is due to the position of two quasars, one at each edge of the filament connecting the two galaxies, with much more redshift than either galaxy.
References
[edit]- ^ a b c d e f g h i j k "Results for object NGC 7603". NASA/IPAC Extragalactic Database. Retrieved 2017-07-06.
- ^ "NGC 7603". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 6 July 2017.
- ^ "Revised NGC Data for NGC 4889". spider.seds.org. Retrieved 2015-10-13.
- ^ "ARP Atlas of Peculiar Galaxies 89-92". ARP ATLAS OF PECULIAR GALAXIES. Retrieved 7 July 2017.
- ^ "NGC 7603". Quasars.org. Archived from the original on 12 October 2018. Retrieved 3 December 2018.
- ^ "Universe: The Cosmology Quest 1 of 2". Youtube. Retrieved 3 December 2018.
External links
[edit]
Media related to NGC 7603 at Wikimedia Commons- SEDS – NGC 7603
- Simbad – NGC 7603
- VizieR – NGC 7603
- NGC 7603 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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