| IC 1613 | |
IC 1613 on DSS2, 0.3° view |
|
| Observation data (J2000 epoch) | |
|---|---|
| Constellation | Cetus |
| Right ascension | 01h 04m 47.8s[1] |
| Declination | +02° 07' 04"[1] |
| Redshift | -234 ± 1 km/s[1] |
| Distance | 2.38 ± 0.07 Mly (730 ± 20 kpc)[2][3] |
| Type | IB(s)m[1] |
| Apparent dimensions (V) | 16′.2 × 14′.5[1] |
| Apparent magnitude (V) | 9.9[1] |
| Notable features | - |
| Other designations | |
| UGC 668,[1] DDO 8,[1] PGC 3844[1] | |
| See also: Galaxy, List of galaxies | |
IC 1613 is an irregular galaxy and a dwarf galaxy in the Cetus constellation near 26 Ceti.[4] It was discovered in 1906 by Max Wolf,[4] and is approaching earth at 234 km/s.
IC 1613 is a member of our Local Group.[4] It has played an important role in the calibration of the Cepheid variable period luminosity relation for estimating distances.[4] Other than the Magellanic Clouds, it is the only Local Group dwarf irregular galaxy where RR Lyrae-type variables have been observed.[4]
In 1999, Cole et al.[4] used the Hubble Space Telescope to find that the dominant population of this galaxy has an age of ~7 Gyr. Using its Hess diagram, they found that its evolutionary history may be similar to that of the Pegasus dIrr. Both galaxies are classified as Ir V in the DDO system. Also in 1999, Antonello et al. found five cephids of Population II in IC 1613, giving self-evident support for the existence of a very old stellar population component of IC 1613. In 1999, King, Modjaz, & Li discovered the first supernova ever detected in IC 1613.[5]
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