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NGC 6503

Coordinates:Sky map17h 49.4m 00s, +70° 09′ 00″
From Wikipedia, the free encyclopedia
Spiral galaxy in the constellation Draco
NGC 6503
HST image of NGC 6503's spiral arms[1]
Observation data (J2000epoch)
ConstellationDraco
Right ascension17h 49m 26.4207s[2]
Declination+70° 08′ 39.587″[2]
Redshift0.000143[3]
Heliocentric radial velocity28[4] km/s
Distance20.9 ± 2.2 Mly (6.40 ± 0.66 Mpc)[4]
Apparent magnitude (V)10.2[5]
Characteristics
TypeSAB:(s)bc[6]
Apparent size (V)7.1 × 2.4[7]
Other designations
IRAS 17499+7009,2MASX J17492651+7008396,UGC 11012,LEDA 60921,MCG +12-17-009[3]

NGC 6503 is afield[8]dwarf spiral galaxy[dubiousdiscuss] in the northernconstellation ofDraco. It was discovered by German astronomerArthur von Auwers on July 22, 1854.[5] The galaxy has anangular size of7.1 × 2.4[7] and anapparent visual magnitude of 10.2.[5] It is located at the distance of 18 millionlight years away from theMilky Way galaxy.[4] NGC 6503 may form the remote tip of a long chain of galaxies that extends out into theLocal Void, forming agalaxy filament spanning 26 millionlight-years (8 Mpc).[9]

Thegalactic plane of this galaxy isinclined at an angle of78°± to theplane of the sky,[4] with themajor axis of its oval profile being aligned along aposition angle of 121°.[10] Themorphological classification of NGC 6502 is SAB:(s)bc. This indicates abarred spiral galaxy (SAB:) with no inner ring structure (s) and moderately woundspiral arms (bc). However, the ':' notation indicates some uncertainty about the classification. Older works gave it a class of SA(s)bc; i.e. no bar.[6]

A possible bar system has been reported viainfrared observations, being viewed end-on from the perspective of the Earth.[11][12]Ultraviolet observations show a young, innerstar forming ring encircling the bar.[12] The ring has a radius between 1 and 2.5 kpc from the core.[13] There is a disk of neutral hydrogen that is larger in extent than the optical disk of the galaxy. This extra-planar gas is mostly the result of star formation activity, rather than cold gas that is being accreted.[14] There is evidence for aLINER-type orSeyfert 2 nucleus.[12]

NGC 6503 has one knownsatellite galaxy,[15] known as KK 242. With a stellar mass of about 3 millionsolar masses, KK 242 is on the border between a dwarfirregular galaxy (dIrr) and adwarf spheroidal galaxy (dSph).[16]

Gallery

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References

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  1. ^"NGC 6503".space telescope.org. NASA/ESA. Retrieved11 June 2015.
  2. ^abBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  3. ^ab"NGC 6503".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2010-11-29.
  4. ^abcdKourkchi, Ehsan; et al. (October 23, 2020)."Cosmicflows-4: The Catalog of ∼10,000 Tully–Fisher Distances".The Astrophysical Journal.902 (2): 145.arXiv:2009.00733.Bibcode:2020ApJ...902..145K.doi:10.3847/1538-4357/abb66b.ISSN 1538-4357.
  5. ^abcO'Meara, Stephen James (2007).Hidden Treasures. Cambridge University Press. p. 423.ISBN 978-1-139-46373-7.
  6. ^abButa, Ronald J.; et al. (2015). "A Classical Morphological Analysis of Galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G)".The Astrophysical Journal Supplement Series.217 (2): 32.arXiv:1501.00454.Bibcode:2015ApJS..217...32B.doi:10.1088/0067-0049/217/2/32.S2CID 119202943.
  7. ^abBlanc, Guillermo A.; et al. (2013). "The Virus-P Exploration of Nearby Galaxies (Venga): Survey Design, Data Processing, and Spectral Analysis Methods".The Astronomical Journal.145 (5): 138.arXiv:1303.1552.Bibcode:2013AJ....145..138B.doi:10.1088/0004-6256/145/5/138.S2CID 119109864.
  8. ^Materne, J. (April 1979). "The structure of nearby groups of galaxies - Quantitative membership probabilities".Astronomy and Astrophysics.74 (2):235–243.Bibcode:1979A&A....74..235M.
  9. ^Karachentseva, Valentina E.; et al. (October 2023). "The M 101 galaxy group as a node in a nearby cosmic filament".Astronomy & Astrophysics.678. id. A16.arXiv:2308.01897.Bibcode:2023A&A...678A..16K.doi:10.1051/0004-6361/202347085.
  10. ^Bottema, Roelof; Gerritsen, Jeroen P. E. (October 1997)."An investigation of the structure and kinematics of the spiral galaxy NGC 6503".Monthly Notices of the Royal Astronomical Society.290 (4):585–597.arXiv:astro-ph/9704190.doi:10.1093/mnras/290.4.585.
  11. ^Kuzio de Naray, Rachel; et al. (December 2012)."Searching for non-axisymmetries in NGC 6503: a weak end-on bar".Monthly Notices of the Royal Astronomical Society.427 (3):2523–2536.arXiv:1209.4653.Bibcode:2012MNRAS.427.2523K.doi:10.1111/j.1365-2966.2012.22126.x.
  12. ^abcFreeland, E.; Chomiuk, L.; Keenan, R.; Nelson, T. (March 2010). "Evidence for a Strong End-On Bar in the Ringed σ-Drop Galaxy NGC 6503".The Astronomical Journal.139 (3):865–870.arXiv:0912.0247.Bibcode:2010AJ....139..865F.doi:10.1088/0004-6256/139/3/865.
  13. ^Gouliermis, Dimitrios A.; et al. (October 2015)."Hierarchical star formation across the ring galaxy NGC 6503".Monthly Notices of the Royal Astronomical Society.452 (4):3508–3528.arXiv:1506.03928.Bibcode:2015MNRAS.452.3508G.doi:10.1093/mnras/stv1325.
  14. ^Greisen, Eric W.; et al. (June 2009). "Aperture Synthesis Observations of the Nearby Spiral NGC 6503: Modeling the Thin and Thick H I Disks".The Astronomical Journal.137 (6):4718–4733.arXiv:0902.0989.Bibcode:2009AJ....137.4718G.doi:10.1088/0004-6256/137/6/4718.
  15. ^Koda, Jin; et al. (April 2015). "Discovery of New Dwarf Galaxy Near the Isolated Spiral Galaxy NGC 6503".The Astrophysical Journal Letters.802 (2). id. L24.arXiv:1504.00674.Bibcode:2015ApJ...802L..24K.doi:10.1088/2041-8205/802/2/L24.
  16. ^Karachentsev, Igor D.; et al. (2022)."KK 242, A Faint Companion to the Isolated SCD Galaxy NGC 6503".The Astronomical Journal.163 (2): 51.arXiv:2111.14691.Bibcode:2022AJ....163...51K.doi:10.3847/1538-3881/ac3cbe.S2CID 244714422.

Further reading

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