From Wikipedia, the free encyclopedia
ESO 306-17
Image of ESO 306-17 by the Hubble Space Telescope
Release date: 4 March 2010
Observation data ( J2000.0 epoch)
Constellation Columba
Right ascension05h 40m 06.73s [1]
Declination−40° 50′ 10.6″ [1]
Redshift0.035805±0.000083 [2]
Heliocentric radial velocity10,734±25  km/s [2]
Galactocentric velocity10,544±26  km/s [2]
Distance517.3 ± 36.20  Mly (158.6 ± 11.1  Mpc)h−1
0.6774

(Comoving) [2]
506  Mly (155.1  Mpc)h−1
0.6774

( Light-travel)
Apparent magnitude (B)13.36 [1]
Characteristics
TypeE+3 [2]
Size1,070,000  ly × 706,100 ly
(328.04  kpc × 216.50 kpc)
( diameter; 90% total B-band light) [2] [a]
399,300  ly × 287,500 ly
(122.42  kpc × 88.15 kpc)
( diameter; "total" magnitude) [2] [a]
Apparent size (V)2.5 × 1.5 ( V-band) [2]
Other designations
MCG -07-12-009, PGC 17570 [3]

ESO 306-17 is a fossil group giant elliptical galaxy in the Columba constellation, about 1.07 million light-years in diameter, [2] [4] and roughly 517 million light-years away. [2]

The galaxy is situated alone in a volume of space about it. It is theorized that the galaxy cannibalized its nearest companions, hence, being a fossil group. [5] The galaxy is a giant elliptical of type cD3 [2] (E+3), one of the largest types of galaxies.

Notes

  1. ^ a b The quoted diameter in this infobox was based on NED's provided scale " Virgo + GA + Shapley" of 769 pc/arcsec multiplied with given angular diameters.

References

  1. ^ a b c "Search specification: ESO 306-17". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-13.
  2. ^ a b c d e f g h i j k "Results for object NGC ESO 306-17 (ESO 306-17)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-02-13.
  3. ^ "ESO 306-17". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-13.
  4. ^ MSNBC, "A Giant Among Galaxies ?", Alan Boyle, 4 March 2010 (accessed 5 March 2010)
  5. ^ Astronomy Now, "Bully galaxy rules the neighbourhood", Emily Baldwin, 4 March 2010 (accessed 5 March 2010)

External links


From Wikipedia, the free encyclopedia
ESO 306-17
Image of ESO 306-17 by the Hubble Space Telescope
Release date: 4 March 2010
Observation data ( J2000.0 epoch)
Constellation Columba
Right ascension05h 40m 06.73s [1]
Declination−40° 50′ 10.6″ [1]
Redshift0.035805±0.000083 [2]
Heliocentric radial velocity10,734±25  km/s [2]
Galactocentric velocity10,544±26  km/s [2]
Distance517.3 ± 36.20  Mly (158.6 ± 11.1  Mpc)h−1
0.6774

(Comoving) [2]
506  Mly (155.1  Mpc)h−1
0.6774

( Light-travel)
Apparent magnitude (B)13.36 [1]
Characteristics
TypeE+3 [2]
Size1,070,000  ly × 706,100 ly
(328.04  kpc × 216.50 kpc)
( diameter; 90% total B-band light) [2] [a]
399,300  ly × 287,500 ly
(122.42  kpc × 88.15 kpc)
( diameter; "total" magnitude) [2] [a]
Apparent size (V)2.5 × 1.5 ( V-band) [2]
Other designations
MCG -07-12-009, PGC 17570 [3]

ESO 306-17 is a fossil group giant elliptical galaxy in the Columba constellation, about 1.07 million light-years in diameter, [2] [4] and roughly 517 million light-years away. [2]

The galaxy is situated alone in a volume of space about it. It is theorized that the galaxy cannibalized its nearest companions, hence, being a fossil group. [5] The galaxy is a giant elliptical of type cD3 [2] (E+3), one of the largest types of galaxies.

Notes

  1. ^ a b The quoted diameter in this infobox was based on NED's provided scale " Virgo + GA + Shapley" of 769 pc/arcsec multiplied with given angular diameters.

References

  1. ^ a b c "Search specification: ESO 306-17". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-13.
  2. ^ a b c d e f g h i j k "Results for object NGC ESO 306-17 (ESO 306-17)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-02-13.
  3. ^ "ESO 306-17". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-13.
  4. ^ MSNBC, "A Giant Among Galaxies ?", Alan Boyle, 4 March 2010 (accessed 5 March 2010)
  5. ^ Astronomy Now, "Bully galaxy rules the neighbourhood", Emily Baldwin, 4 March 2010 (accessed 5 March 2010)

External links



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