Cannabaceae

NGC 3206
The barred spiral galaxy NGC 3206.
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension10h 21m 47.5922s[1]
Declination+56° 55′ 49.519″[1]
Redshift0.003839 [1]
Heliocentric radial velocity1151 ± 1 km/s[1]
Distance63.0 ± 4.4 Mly (19.31 ± 1.36 Mpc)[1]
Apparent magnitude (V)11.9[1]
Characteristics
TypeSB(s)cd[1]
Size~50,000 ly (15.34 kpc) (estimated)[1]
Apparent size (V)2.9' x 1.9'[1]
Other designations
IRAS 10184+5710, 2MASX J10214758+5655494, UGC 5589, MCG +10-15-069, PGC 30322, CGCG 290-030[1]

NGC 3206 is a barred spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background is 1309 ± 11 km/s, which corresponds to a Hubble distance of 19.31 ± 1.36 Mpc (∼63 million light-years).[1] In addition, 11 non redshift measurements give a distance of 17.582 ± 1.088 Mpc (~57.3 million light-years).[2] The galaxy was discovered by German-British astronomer William Herschel on 8 April 1793.[3]

According to the SIMBAD database, NGC 3206 is an Active Galaxy Nucleus Candidate, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.[4]

One supernova has been observed in NGC 3206: on 29 January 2024, American amateur astronomer Patrick Wiggins discovered SN 2024bch (type II, mag. 16.1).[5]

NGC 3264 Group

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NGC 3206 is part of the NGC 5908 group (also known as LGG 201), which includes at least five other members: NGC 3220, NGC 3264, NGC 3353, UGC 5848, and UGCA 211.[6]

See also

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References

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  1. ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 3206. Retrieved 15 August 2024.
  2. ^ "Distance Results for NGC 3206". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 15 August 2024.
  3. ^ Seligman, Courtney. "NGC 3206". Celestial Atlas. Retrieved 15 August 2024.
  4. ^ "NGC 5876". SIMBAD astronomical database. Strasbourg Astronomy Data Centre. Retrieved 15 August 2024.
  5. ^ "SN 2024bch". Transient Name Server. IAU. Retrieved 15 August 2024.
  6. ^ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
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One thought on “Cannabaceae

  1. Well, that’s interesting to know that Psilotum nudum are known as whisk ferns. Psilotum nudum is the commoner species of the two. While the P. flaccidum is a rare species and is found in the tropical islands. Both the species are usually epiphytic in habit and grow upon tree ferns. These species may also be terrestrial and grow in humus or in the crevices of the rocks.
    View the detailed Guide of Psilotum nudum: Detailed Study Of Psilotum Nudum (Whisk Fern), Classification, Anatomy, Reproduction

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