NGC 1569
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| NGC 1569 | |
 A Hubble Space Telescope (HST) image of NGC 1569. Credit: HST/NASA/ESA. |
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| Observation data (J2000 epoch) | |
|---|---|
| Constellation | Camelopardalis |
| Right ascension | 4h 30m 49.1s[1] |
| Declination | +64° 50′ 53″[1] |
| Redshift | -104 km/s[1] |
| Distance | 7.8 ± 2.0 Mly (2.4 ± 0.6 Mpc)[2] |
| Type | IBm[1] |
| Apparent dimensions (V) | 3′.6 × 1′.8[1] |
| Apparent magnitude (V) | 11.9[1] |
| Notable features | Contains two super star clusters |
| Other designations | |
| UGC 3056,[1] PGC 15345,[1] VII Zw 016,[1] Arp 210[1] |
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| See also: Galaxy, List of galaxies | |
NGC 1569 is a dwarf irregular galaxy in Camelopardalis. While this faint galaxy is not a popular amateur astronomy target, it is well studied by professional astronomers, who are interested in the history of star formation within the galaxy. The galaxy is relatively nearby; the distance to the galaxy is only 2.4 Mpc (7.8 Mly).[2] Consequently, the Hubble Space Telescope can easily resolve the stars within the galaxy.[3]
Contents |
[edit] Star formation
NGC 1569 contains two prominent super star clusters with different histories.[3][4] Both clusters have experienced episodic star formation. Super star cluster A, located in the northwest of the galaxy, contains young stars (including Wolf-Rayet stars) that formed less than 5 million years ago as well as older red stars[4][5]. Super star cluster B, located near the center of the galaxy, contains an older stellar population of red giants and red supergiants[4][3][5]. Both of these star clusters are thought to have masses equivalent to the masses of the globular clusters in the Milky Way. Numerous smaller star clusters with relatively young ages have also been identified[3]. These results, along with the results from other dwarf galaxies such as the Large Magellanic Cloud and NGC 1705, demonstrate that star formation in dwarf galaxies does not occur continuously but instead occurs in a series of short, nearly instantaneous bursts.
[edit] Blueshift
NGC 1569 is exceptional in that its spectrum is blueshifted.[1] This means that the galaxy is moving towards the Earth. In contrast, the spectra of most other galaxies are redshifted because of the expansion of the universe.
[edit] References
- ^ a b c d e f g h i j k NASA/IPAC Extragalactic Database. Results for NGC 1569. Retrieved on 2007-03-15.
- ^ a b Makarova, L. N.; Karachentsev, I. D. (2003). "On the Distance to Nearby Dwarf Galaxy NGC 1569". Astrophysics (English translation of Astrofizika) 46 (2): 144–150.
- ^ a b c d D. A. Hunter, R. W. O'Connell, J. S. Gallagher, T. A. Smecker-Hane (2000). "The Star Clusters in the Starburst Irregular Galaxy NGC 1569". Astronomical Journal 120: 2383–2401. doi:.
- ^ a b c L. Origlia, C. Leitherer, A. Aloisi, L. Greggio, M. Tosi (2001). "The Stellar Content of the Super-Star Clusters in NGC 1569". Astronomical Journal 122: 815–824. doi:.
- ^ a b G. J. Bendo, R. D. Joseph (2004). "Nuclear Stellar Populations in the Infrared Space Observatory Atlas of Bright Spiral Galaxies". Astronomical Journal 127: 3338–3360. doi:.
[edit] External links
- NGC 1569 at ESA/Hubble
- The NGC 1569 on the WikiSky: DSS2, SDSS, IRAS, Hidrogen α, X-Ray, Astrophoto, Sky Map
