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KKR 03

In today's world, KKR 03 has become a topic of constant interest and debate. Whether it's its impact on society, its historical relevance, or its influence on popular culture, KKR 03 attracts the attention of people of all ages, genders, and backgrounds. Over the years, KKR 03 has generated all kinds of opinions, theories and interpretations, becoming a central element in numerous areas. In this article, we will explore different aspects of KKR 03 and its meaning in the contemporary context. From its origin to its current repercussions, we will take an in-depth look at the importance of KKR 03 in our world today.

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KKR 03
Observation data (J2000 epoch)
ConstellationCanes Venatici
Right ascension14h 07m 10.7s[1]
Declination+35° 03′ 37″[1]
Redshift0.000211[2]
Heliocentric radial velocity63.3 ± 1.8 km/s (39.3 ± 1.1 mi/s)[2]
Distance6.4 million ly (1.97 million pc)[1]
Apparent magnitude (V)15.68[3]
Absolute magnitude (V)−10.85[3]
Characteristics
TypedIrr[2]
Size980 ly (300 pc)[1]
Other designations
LEDA 166185, PGC 166185, 140501.5+351809, 230, 384.4, 3, 11HUGS 367, MAPS-NGP O_271_0183623

KKR 03 is a dwarf irregular galaxy located 6.4 million light-years (1.97 million parsecs) away from Earth.[1] It has an absolute magnitude of −10.85[3] and lies on the inner edge of the M94 Group.[4]

See also

References

  1. ^ a b c d e Dalcanton, Julianne J.; Williams, Benjamin F.; Seth, Anil C.; Dolphin, Andrew; Holtzman, Jon; et al. (July 2009). "The ACS Nearby Galaxy Survey Treasury". The Astrophysical Journal Supplement. 183 (1): 67–108. arXiv:0905.3737. Bibcode:2009ApJS..183...67D. doi:10.1088/0067-0049/183/1/67. S2CID 5032304.
  2. ^ a b c McConnachie, Alan W. (July 2012). "The Observed Properties of Dwarf Galaxies in and around the Local Group". The Astronomical Journal. 144 (1). 4. arXiv:1204.1562. Bibcode:2012AJ....144....4M. doi:10.1088/0004-6256/144/1/4. S2CID 118515618.
  3. ^ a b c Sharina, M. E.; Karachentsev, I. D.; Dolphin, A. E.; Karachentseva, V. E.; Tully, R. Brent; et al. (March 2008). "Photometric properties of the Local Volume dwarf galaxies". Monthly Notices of the Royal Astronomical Society. 384 (4): 1544–1562. arXiv:0712.1226. Bibcode:2008MNRAS.384.1544S. doi:10.1111/j.1365-2966.2007.12814.x. S2CID 119199602.
  4. ^ Karachentsev, I. D.; Kashibadze, O. G.; Makarov, D. I.; Tully, R. B. (March 2009). "The Hubble flow around the Local Group". Monthly Notices of the Royal Astronomical Society. 393 (4): 1265–1274. arXiv:0811.4610. Bibcode:2009MNRAS.393.1265K. doi:10.1111/j.1365-2966.2008.14300.x. S2CID 13912040.