Jump to content

Messier 35: Difference between revisions

Coordinates: Sky map 06h 09.1m 00s, 24° 21′ 00″
From Wikipedia, the free encyclopedia
Content deleted Content added
Added info on NGC 2158
Line 37: Line 37:
| doi =10.1086/167287
| doi =10.1086/167287
}}</ref> The mass within the central 3.75 [[parsec]]s was found to be between 1600 and 3200 solar masses (95 percent confidence), consistent with the mass of a realistic stellar population within the same radius.
}}</ref> The mass within the central 3.75 [[parsec]]s was found to be between 1600 and 3200 solar masses (95 percent confidence), consistent with the mass of a realistic stellar population within the same radius.

The compact open cluster [[NGC 2158]] lies directly southwest of M 35.


==See also==
==See also==

Revision as of 07:08, 3 January 2013

Messier 35
Credit: 2MASS/NASA.
Object typeOpen cluster Edit this on Wikidata
Other designationsNGC 2168[1]
Observation data
(Epoch J2000)
ConstellationGemini
06h 09.1m [1]
Declination+24° 21′[1]
Distance2800 ly / 850 pc

In visual light (V)
5.30
Unknown
Size
28 arcmins

Radiusunknown
Related media on Wikimedia Commons

Messier 35 (also known as M 35, or NGC 2168) is an open cluster in the constellation Gemini. It was discovered by Philippe Loys de Chéseaux in 1745 and independently discovered by John Bevis before 1750. The cluster is scattered over an area of the sky almost the size of the full moon and is located 850 parsecs (2,800 light-years) from Earth.

The mass of M35 has been computed using a statistical technique based on proper motion velocities of its stars.[2] The mass within the central 3.75 parsecs was found to be between 1600 and 3200 solar masses (95 percent confidence), consistent with the mass of a realistic stellar population within the same radius.

The compact open cluster NGC 2158 lies directly southwest of M 35.

See also

References

  1. ^ a b c "SIMBAD Astronomical Database". Results for Messier 35. Retrieved 8 December 2006.
  2. ^ Leonard, P. J. T.; Merritt, D. (1989). "The mass of the open star cluster M35 as derived from proper motions". Astrophysical Journal. 339 (1): 195–208. Bibcode:1989ApJ...339..195L. doi:10.1086/167287.