NGC 2438

NGC 2438

NGC 2438 and the Calabash Nebula
Observation data
(Epoch J2000.0)
Right ascension 07h 41.8m
Declination -14° 44
Distance 2,900 ly
Apparent magnitude (V) +10.8
Apparent dimensions (V) 1.1 arcmins
Constellation Puppis
Physical characteristics
Radius -
Absolute magnitude (V) -
Notable features Superimposed
on Messier 46
Other designations H IV.39, FC 87, PK 231+4.2

NGC 2438 is a planetary nebula about 3,000 light years away in the constellation Puppis.[1] It was discovered by William Herschel on March 19, 1786.[2] The planetary nebula NGC 2438 appears to lie within the cluster M46, but it is most likely unrelated since it does not share the cluster's radial velocity.[3][4] The case is yet another example of a superposed pair, joining the famed case of NGC 2818.[3][5]

Long exposures have shown that this planetary nebula has an extended halo,[6] while the more easily visible portion probably dates to the death of the red giant in its center.[2]

Central star

The central star of this planetary nebula is a 17.7-magnitude white dwarf,[2] with surface temperature of about 75,000 K (74,700 °C).[7] It is one of the hottest stars known.

See also

References

  1. "Astronomy Picture of the Day, Planetary Nebula NGC 2438". NASA. 2011-04-07. Retrieved 2011-04-08.
  2. 1 2 3 "NGC Objects: NGC 2400 - 2449". Retrieved 2011-04-08.
  3. 1 2 Majaess D. J., Turner D., Lane D. (2007). In Search of Possible Associations between Planetary Nebulae and Open Clusters, PASP, 119, 1349
  4. Kiss, L. L., Szabó, Gy. M., Balog, Z., Parker, Q. A., Frew, D. J. (2008). AAOmega radial velocities rule out current membership of the planetary nebula NGC 2438 in the open cluster M46, MNRAS
  5. Mermilliod, J.-C., Clariá, J. J., Andersen, J., Piatti, A. E., Mayor, M. (2001). Red giants in open clusters. IX. NGC 2324, 2818, 3960 and 6259, A&A
  6. "NGC 2438". SEDS. Retrieved 2011-04-08.
  7. "Planetary Nebula NGC 2438 in Puppis". Retrieved 2011-04-08.

External links

Coordinates: 07h 41m 50.6s, −14° 44′ 05″

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