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NGC 5907

Coordinates:Sky map15h15m53.8s,+56° 19′ 44″
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NGC5907
NGC 5907
Observation data (J2000epoch)
ConstellationDraco
Right ascension15h15m53.8s[1]
Declination+56° 19′ 44″[1]
Redshift0.002225[1]
Heliocentric radial velocity667 ± 3km/s[1]
Distance53.5 ± 8.1 Mly
(16.4 ± 2.5 Mpc)[2]
Apparent magnitude(V)11.1[1]
Characteristics
TypeSA(s)c:
Apparent size(V)12.7' x 1.4'[1]
Other designations
H II.759, GC 4087, h 1917, Splinter Galaxy, NGC 5906, UGC 09801, PGC 054470, MCG +09-25-040[1]

NGC 5907(also known asKnife Edge GalaxyorSplinter Galaxy) is aspiral galaxylocated approximately 50 millionlight yearsfromEarth.[2]William Herscheldiscovered the galaxy in 1788.

Characteristics

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NGC 5907 has an anomalously lowmetallicityand few detectablegiant stars,being apparently composed almost entirely ofdwarf stars.[3]It is a member of theNGC 5866 Group.

NGC 5907 has long been considered a prototypical example of a warped spiral in relative isolation. In 2006, an international team of astronomers announced the presence of an extended tidal stream surrounding the galaxy that challenges this picture and suggests the gravitational perturbations induced by the stream progenitor may be the cause for the warp. The existence of part of these tidal streams has been recently challenged by some deeper surveys.

Onesupernovahas been observed in NGC 5907: SN 1940A (type unknown, mag 14.3).[4][5]

Anultraluminous X-ray sourceis located in the galaxy.[6]

Location

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The edge-on galaxy is seen in the constellation Draco, near the stariota Draconis.It is seen in the sky near to the much more distant galaxyNGC 5965.

NGC Identification

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NGC 5907 is also known as NGC 5906.[7][8]This second NGC number refers to a fainter part of the galaxy[7]lying west of the dust lane[8]that was recorded by astronomer and physicistGeorge Johnstone Stoneyon April 13, 1850.[7]

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References

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  1. ^abcdefg"NASA/IPAC Extragalactic Database".Results for NGC 5907.Retrieved2010-07-11.
  2. ^ab"Distance Results for NGC 5907".NASA/IPAC Extragalactic Database.Retrieved2010-07-11.
  3. ^Liu, M. C.; Marleau, F. R.; Graham, J. R.; Charlot, S.; Sackett, P.; Zepf, S. E. (December 1998). "Weighing the Stellar Content of NGC 5907's Dark Matter Halo".Bulletin of the American Astronomical Society.30:1258.Bibcode:1998AAS...193.0807L.
  4. ^"List of Supernovae".Harvard-Smithsonian Center for Astrophysics (IAU).Retrieved2010-07-11.
  5. ^Transient Name Server entry for SN 1940A.Retrieved 28 March 2023.
  6. ^Israel, Gian Luca; Belfiore, Andrea; Stella, Luigi; Esposito, Paolo; Casella, Piergiorgio; De Luca, Andrea; Marelli, Martino; Papitto, Alessandro; Perri, Matteo; Puccetti, Simonetta; Rodríguez Castillo, Guillermo A.; Salvetti, David; Tiengo, Andrea; Zampieri, Luca; D’Agostino, Daniele; Greiner, Jochen; Haberl, Frank; Novara, Giovanni; Salvaterra, Ruben; Turolla, Roberto; Watson, Mike; Wilms, Joern; Wolter, Anna (24 Feb 2017). "An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907".Science.355(6327): 817–819.arXiv:1609.07375.Bibcode:2017Sci...355..817I.doi:10.1126/science.aai8635.PMID28219970.S2CID206653306.
  7. ^abc"New General Catalog Objects: NGC 5900 - 5949".cseligman.Retrieved2020-06-26.
  8. ^ab"Your NED Search Results".ned.ipac.caltech.edu.Retrieved2020-06-26.
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