Astronomy:NGC 4013
| NGC 4013 | |
|---|---|
 HST closeup view of NGC 4013 | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 11h 58m 31.13s[1] |
| Declination | +43° 56′ 50.1″[1] |
| Redshift | 831 ± 1 km/s[1] |
| Distance | 60.6 ± 8.1 Mly (18.6 ± 2.5 Mpc)[2] |
| Apparent magnitude (V) | 12.1B[1] |
| Characteristics | |
| Type | SBa[1] |
| Apparent size (V) | 5.2' x 1.0'[1] |
| Other designations | |
| UGC 6963,[1] PGC 37691[1] LEDA 37691[3] 2MFGC 9412[3]
IRAS 11559+4413[3] 2MASX J11583141+4356492[3] MCG+07-25-009[3] UZC J115831.5+435651[3] | |
NGC 4013 is an edge-on barred spiral galaxy about 55 million light-years away in the constellation Ursa Major. The disk of NGC 4013 shows a distinct "peanut"-shaped bulge in long exposure photographs that N-body computer simulations suggest is consistent with a stellar bar seen perpendicular to the line of sight.[4]
A recent deep color image of NGC 4013 revealed a looping tidal stream of stars extending over 80 thousand light-years from the Galactic Center. This structure is thought to be the remnants of a smaller galaxy that was torn apart by tidal forces as it collided with NGC 4013.[5]
Supernova SN 1989Z was discovered on December 30, 1989 at apparent magnitude 12.[6]
NGC 4013 is a member of the Ursa Major Cluster.[7]
See also
- Cigar Galaxy
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 "NASA/IPAC Extragalactic Database". Results for NGC 4013. http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=NGC+4013&img_stamp=yes&extend=no.
- ↑ "Distance Results for NGC 4013". NASA/IPAC Extragalactic Database. http://nedwww.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+4013.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 "SIMBAD". Results for NGC 4013. http://simbad.harvard.edu/simbad/sim-basic?Ident=NGC+4013&submit=SIMBAD+search.
- ↑ Combes, F. and Sanders, R.H., "Formation and properties of persisting stellar bars", Astronomy and Astrophysics, vol. 96, no. 1-2, Mar. 1981, p. 164-173.
- ↑ D. Martínez-Delgado (IAC); M. Pohlen (Cardiff); R. Jay GaBany (Blackbird Obs); S. Majewski (Univ Virginia) et al. (2009). "Discovery of a Giant Stellar Tidal Stream Around the Disk Galaxy NGC 4013". Astrophysical Journal 692 (2): 955–963. doi:10.1088/0004-637X/692/2/955. Bibcode: 2009ApJ...692..955M. http://www.iop.org/EJ/abstract/0004-637X/692/2/955.
- ↑ "List of Supernovae". Harvard-Smithsonian Center for Astrophysics (IAU). http://cbat.eps.harvard.edu/lists/Supernovae.html#1989Z.
- ↑ Rueff, Katherine M.; Howk, J. Christopher; Pitterle, Marissa; Hirschauer, Alec S.; Fox, Andrew J.; Savage, Blair D. (2013-01-31). "The Relationship Between the Dense Neutral and Diffuse Ionized Gas in the Thick Disks of Two Edge-On Spiral Galaxies". The Astronomical Journal 145 (3): 62. doi:10.1088/0004-6256/145/3/62. ISSN 0004-6256. Bibcode: 2013AJ....145...62R. http://stacks.iop.org/1538-3881/145/i=3/a=62?key=crossref.4248e4d9cf6487e6f1fc7dd4df72a8c2.
External links
- The Discovery of a Giant Stellar Tidal Stream Around NGC4013
- HubbleSite NewsCenter: A Galaxy on the Edge
- NASA Astronomy Picture of the Day: NGC 4013 and the Tidal Stream (7 February 2008)
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