Astronomy:NGC 6789

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Short description: Irregular galaxy in the constellation Draco
NGC 6789
NGC 6789 hst 09162 R814B606.png
Hubble Space Telescope image of NGC 6789
Observation data (J2000 epoch)
ConstellationDraco
Right ascension 19h 16m 41s[1]
Declination+63° 58′ 23″[1]
Redshift−0.000470[2]
Helio radial velocity−141 ± 9 km/s[2]
Distance12 Mly (3.6 Mpc)[3]
Apparent magnitude (B)13.76[1]
Characteristics
TypeIm[2]
Other designations
NGC 6789,MCG+11-23-001, LEDA 63000[1]

NGC 6789 is a void[4] irregular galaxy in the constellation Draco. It was discovered by Lewis Swift on Aug 30, 1883.[5] It is located within the Local Void, a region of space with far fewer galaxies than its surroundings.[4]

NGC 6789 is the nearest blue compact dwarf (BCD) galaxy to the Milky Way. It is chemically homogeneous and relatively metal-poor.[3]

See also

References

  1. 1.0 1.1 1.2 1.3 "NGC 6789". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+6789. 
  2. 2.0 2.1 2.2 "NASA/IPAC Extragalactic Database". http://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=47146&objname=1&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1#BasicData_0. 
  3. 3.0 3.1 García-Benito, R.; Pérez-Montero, E. (2012). "Auto-consistent metallicity and star formation history of the nearest blue compact dwarf galaxy NGC 6789". Monthly Notices of the Royal Astronomical Society 423 (1): 406–421. doi:10.1111/j.1365-2966.2012.20885.x. Bibcode2012MNRAS.423..406G. 
  4. 4.0 4.1 Lelli, Federico; Verheijen, Marc; Fraternali, Filippo (2014). "The triggering of starbursts in low-mass galaxies". Monthly Notices of the Royal Astronomical Society 445 (2): 1694–1712. doi:10.1093/mnras/stu1804. Bibcode2014MNRAS.445.1694L. 
  5. Seligman, Courtney. "New General Catalog Objects: NGC 6750 - 6799". https://cseligman.com/text/atlas/ngc67a.htm#6789. 

External links