IC 2759 | |
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Observation data | |
Constellation | Leo |
Right ascension | 11h 22m 13.280s |
Declination | +24d 19m 01.80s |
Redshift | 0.025684 |
Heliocentric radial velocity | 7,700 km/s |
Distance | 350 Mly (107 Mpc) |
Group or cluster | Hickson 51 |
Apparent magnitude (V) | 15.5 |
Characteristics | |
Type | E, S0?, E2 |
Size | 42,000 ly |
Other designations | |
PGC 34881, ARK 290, CGCG 126-041, MCG +04-27-027, 2MASX J11221325+2419017, HCG 051E, WBL 326-003, 2CXO J112213.2+241901, 2XMM J112213.1+241900, NSA 139264, 2MASS J11221327+2419023, SDSS J112213.28+241901.7, LEDA 34881 |
IC 2759 is a small type E elliptical galaxy located in the constellation of Leo. [1] [2] [3] It is located 350 million light-years away from the Solar System [4] and was discovered on April 24, 1897, by Guillaume Bigourdan. [5] Sometimes IC 2759 is confused with the spiral galaxy, PGC 34882 which is located south of the galaxy. [6] [7]
One supernova has been discovered in IC 2759 so far: SN 2020lyo.
SN 2020lyo
SN 2020lyo [8] was discovered in IC 2759 by astronomer, Dr. David Bersier [9] on 8 June 2020 from All Sky Automated Survey for SuperNovae (ASAS-SN). [10] via a Liverpool Telescope. [9] It was 0".5 west and 0".0 south of the nucleus and located at redshift of 0.027. [10] The supernova was Type Ia. [8]
IC 2759 is a member of Hickson 51. [11] [12] It was one of the galaxies observed by Paul Hickson, when he published his article in 1982. [13] The other galaxies in Hickson 51, are NGC 3651, PGC 34882, NGC 3653, PGC 34907, PGC 34899 or NGC 3651 NED02 and PGC 34901. [14] IC 2759 in this case, is listed as HCG 51E. [2]
NGC 7038 is an intermediate spiral galaxy located about 210 million light-years away in the constellation of Indus. Astronomer John Herschel discovered NGC 7038 on September 30, 1834.
NGC 3336 is a barred spiral galaxy located about 190 million light-years away in the constellation Hydra. It was discovered by astronomer John Herschel on March 24, 1835. NGC 3336 is a member of the Hydra Cluster.
NGC 1259 is a lenticular galaxy located about 243 million light-years away in the constellation Perseus. The galaxy was discovered by astronomer Guillaume Bigourdan on October 21, 1884 and is a member of the Perseus Cluster.
NGC 1268 is a spiral galaxy located about 140 million light-years away in the constellation Perseus. It was discovered by astronomer Heinrich d'Arrest on February 14, 1863. NGC 1268 is a member of the Perseus Cluster and appears to show signs of distortion in the form of bridges. These features may be the result of a strong interaction with NGC 1267.
NGC 1282 is an elliptical galaxy located about 230 million light-years away in the constellation Perseus. It was discovered by astronomer Guillaume Bigourdan on October 23, 1884. NGC 1282 is a member of the Perseus Cluster.
NGC 3841 is an elliptical or lenticular galaxy located about 300 million light-years away in the constellation Leo. It was discovered by astronomer John Herschel on March 25, 1827 is a member of the Leo Cluster.
NGC 4316 is an edge-on spiral galaxy located about 70 million light-years away in the constellation Virgo. It was discovered by astronomer Wilhelm Tempel on March 17, 1882. NGC 4316 is a member of the Virgo Cluster and is classified as LINER and as a Seyfert galaxy.
UGC 6697 is a large irregular spiral galaxy with a bar located in the Leo constellation. It is located 378 million light-years from the Solar System and has an estimated diameter of 205,000 light-years. UGC 6697 is considered a starburst galaxy which produces high rates of star formation.
NGC 3746 is a large barred spiral galaxy with a ring structure located in the Leo constellation. It is located 449 million light-years from the Solar System and has an approximate diameter of 165,000 light-years. NGC 3746 was discovered by Ralph Copeland on 9 February 1874 with subsequent observations made by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer.
NGC 3750 is a lenticular galaxy with a bar located in the constellation of Leo. It is located 450 million light-years from the Solar System and was discovered by Ralph Copeland on February 9, 1874.
NGC 3748 is a lenticular galaxy with a bar located in the Leo constellation. It is located 440 million light-years away from the Solar System and was discovered by Ralph Copeland on April 5, 1874, but also observed by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer.
NGC 3754 is a small barred spiral galaxy located in Leo. It is located 447 million light-years away from the Solar System and was discovered on April 5, 1874, by Ralph Copeland.
NGC 3745 is a lenticular galaxy with a bar structure located in the constellation of Leo. NGC 3745 is located 471 million light-years away from the Solar System and was discovered by Ralph Copeland on April 5, 1874, but also observed by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer.
NGC 3751 is a type E-S0 lenticular galaxy located in the Leo constellation. It is located 450 million light-years away from the Solar System and was discovered by Ralph Copeland on April 5, 1874.
IC 5145 is a type Sab spiral galaxy located in the constellation Pegasus. It is located 356 million light-years from the Solar System and was discovered by Edward Emerson Barnard, although the year he discovered it is unknown.
NGC 7222 is a large barred spiral galaxy with a ring structure, located in the constellation Aquarius. It is located 570 million light-years away from the Solar System and was discovered by German astronomer, Albert Marth on August 11, 1864.
IC 3275 is a spiral galaxy with a ring structure located in the Virgo constellation. It is located 811 million light-years away from the Solar System and has an approximate diameter of 120,000 light-years across. IC 3275 was discovered on May 7, 1904, by Royal Harwood Frost.
IC 2498 known as PGC 27668, is a type Sb barred spiral galaxy located in constellation Leo. It is located 469 million light-years away from the Solar System and was discovered by Stephane Javelle on April 30, 1896.
IC 1050 is a type Sbc spiral galaxy located in constellation Boötes. It is located 491 million light-years from the Solar System and has an approximate diameter of 130,000 light-years. IC 1050 was discovered by Stephane Javelle on June 3, 1892.
IC 4588 is a type E elliptical galaxy located in the constellation Serpens. It is located 729 million light-years from the Solar System and has a dimension of 0.30 x 0.3 arcmin meaning its diameter is 64,000 light-years across. IC 4588 was discovered by Stephane Javelle on July 15, 1903.