Bear Paw Galaxy (NGC 2537, Arp 6) & IC 2233

NGC 2537 (Arp 6)
NGC 2537 (Arp 6): Galaxy in Ursa Major; 500 mm Cassegrain 3625 mm f/7.2; SBIG STL11K; 300-130-130-130 min LRGB; Bernese Higlands; © 2017 Radek Chromik [32]

History

While looking through his 18.7 inch reflecting telescope William Herschel found on 6 February 1788 an object that he described as follows: «Pretty bright, round, almost of an even light throughout, approaching to planetary, but ill defined and a little fainter on the edges 3/4 or 1' diameter.» He cataloged it as IV 55 (class IV: planetary nebulae: stars with burs, with milky chevelure, with short rays, remarkable shapes, etc.) [464]

In 1833 John Herschel listed this object as h 491 and described it as follows: «Pretty faint; round; 60"; very nearly uniformly bright, but hazy at edges. It is a resolved globular cluster. Being a remarkably fine night, I see the stars; they are 20 m; a star 9.10 mag is 40° south following at distance 2'.» [466] In his «General Catalogue» appeared in 1864 he listed the object a globular cluster with the designation GC 1629. [467] Dreyer took over this mis-classification in his «New General Catalogue» of 1888 where he listed the object as NGC 2537. [313]

In 1966 Halton Arp published his «Atlas of Peculiar Galaxies», where he ordered galaxies into groups based on purely morphological criteria. The galaxy NGC 2537 is listed as Arp 6 in the first group «spiral galaxies, low surface brightness» (group #1-6). [199]

The edge-on galaxy IC 2233 was discovered on 25 March 1894 by the British Astronomer Isaac Robers. He found it by photography, using the 20 inch reflector at his observatory «Starfield», Crowborough Hill, Sussex. [277]

Physical Properties

NGC 2537 is a compact blue dwarf galaxy with a redshift of z=0.001491. According to Simbad estimated distances range from 6.9 to 15 Mpc. The small spiral galaxy NGC 2537A (MCG+08-15-051) four arcminutes to the east shows a redshift of z=0.04001 and therefore is much further away and not associated with its optical neighbour. [145, 582]

NGC 2537
NGC 2537: NGC 2537A (left) and NGC 2537 (reight). Section of Sloan Digitized Sky Survey (SDSS9) [147]
IC 2233
IC 2233: Section of Sloan Digitized Sky Survey (SDSS9) [147]

IC 2233 is a superthin edge-on galaxy with low surface brightness and very low global star formation rate. It shows a redshift of z=0.001868. Simbad lists estimated distances ranging from 10.4 to 14.6 Mpc. Although the galaxy is at a projected distance of 16.7 arcminutes to NGC 2537 they seem not to be a bound pair and most likely lie at different distances. There is also no compelling evidence of a recent minor merger in either IC 2233 or NGC 2537, suggesting that both are examples of small disk galaxies evolving in relative isolation. [145, 582] IC 2233 is surrounded by a compact dark matter halo, which may be responsible for the superthin nature of the stellar disc. [583]

Revised+Historic NGC/IC Version 22/9, © 2022 Dr. Wolfgang Steinicke [277]
Name RA Dec Type bMag vMag B-V SB Dim PA z D(z) MD Dreyer Description Identification, Remarks
NGC 2537 08 13 14.4 +45 59 29 Gx (SBm) 12.3 11.7 0.6 12.6 1.7 × 1.5 162 0.001438 6.07 7.940 globular, pB, pL, R, rrr, st 20 WH IV 55; h 491; GC 1629; UGC 4274; MCG 8-15-50; MK 86; KUG 0809+461; CGCG 236-35; KARA 235; Arp 6; VV 138; Bear claw/paw galaxy
NGC 2537 A 08 13 41.1 +45 59 36 Gx (SBc) 16.0 15.4 0.6 14.2 0.6 × 0.6 0.039976 168.8 globular, pB, pL, R, rrr, st 20 WH IV 55; h 491; GC 1629; MCG 8-15-51
IC 2233 08 13 59.0 +45 44 23 Gx (SBcd) 13.1 12.6 0.5 13.3 4.6 × 0.5 172 0.001801 7.61 13.350 pB, L, E np sf, IV. 55 np UGC 4278; MCG 8-15-52; CGCG 236-36; FGC 730

Finder Chart

The galaxy NGC 2537 is located in constellation Lynx. The best time for observation is November to April, when it is high in the sky during night.

Finder Chart Bear Paw Galaxy (NGC 2537, Arp 6) & IC 2233
Bear Paw Galaxy (NGC 2537, Arp 6) & IC 2233 in constellation Lynx. Charts created using SkySafari 6 Pro and STScI Digitized Sky Survey. Limiting magnitudes: Constellation chart ~6.5 mag, DSS2 close-ups ~20 mag. [149, 160]

Objects Within a Radius of 15°

References

  • [32] Astrofotografie by Radek, Bernie and Dragan; sternwarte.ch
  • [145] SIMBAD astronomical database; simbad.u-strasbg.fr/simbad
  • [147] Aladin Lite; aladin.unistra.fr/AladinLite
  • [149] SkySafari 6 Pro, Simulation Curriculum; skysafariastronomy.com
  • [160] The STScI Digitized Sky Survey; archive.stsci.edu/cgi-bin/dss_form
  • [199] «Atlas Of Peculiar Galaxies», Halton Arp, 1966; Astrophysical Journal Supplement, vol. 14, p.1 (1966); DOI:10.1086/190147; Bibcode:1966ApJS...14....1A; ned.ipac.caltech.edu/level5/Arp/frames.html
  • [277] «Historische Deep-Sky Kataloge» von Dr. Wolfgang Steinicke; klima-luft.de/steinicke (2021-02-17)
  • [313] «A New General Catalogue of Nebulae and Clusters of Stars, being the Catalogue of the late Sir John F.W. Herschel, Bart., revised, corrected, and enlarged» Dreyer, J. L. E. (1888); Memoirs of the Royal Astronomical Society. 49: 1–237; Bibcode:1888MmRAS..49....1D
  • [464] «Catalogue of a second thousand of new nebulae and clusters of stars; with a few introductory remarks on the construction of the heavens» William Herschel, Philosophical Transactions of the Royal Society of London, 1 January 1789; DOI:10.1098/rstl.1789.0021
  • [466] «Observations of nebulæ and clusters of stars, made at Slough, with a twenty-feet reflector, between the years 1825 and 1833» John Frederick William Herschel, Philosophical Transactions of the Royal Society of London, 1 January 1833, Pages: 359-505; DOI:10.1098/rstl.1833.0021
  • [467] «Catalogue of nebulae and clusters of stars» John Frederick William Herschel, Philosophical Transactions of the Royal Society of London, 1 January 1864; DOI:10.1098/rstl.1864.0001; jstor.org/stable/108864
  • [582] «H I Imaging Observations of Superthin Galaxies. II. IC 2233 and the Blue Compact Dwarf NGC 2537» Lynn D. Matthews and Juan M. Uson; The Astronomical Journal, Volume 135, Number 1, 2008; DOI:10.1088/0004-6256/135/1/291
  • [583] «Mass modelling of superthin galaxies: IC5249, UGC7321 and IC2233» Arunima Banerjee, Disha Bapat Monthly Notices of the Royal Astronomical Society, Volume 466, Issue 3, April 2017, Pages 3753–3761, December 2016; DOI:10.1093/mnras/stw3219