Astronomy:M2-42

From HandWiki
Short description: Planetary nebula
Minkowski 2-42 (M2-42)
Emission nebula
Planetary nebula
3D Model of M2-42.png
Observation data: J2000 epoch
Right ascension 18h 22m 32.08s[1]
Declination−24° 09′ 27.7″[1]
Distance30,800 (9444 pc)[1] ly
Apparent magnitude (V)13.9[1]
Apparent dimensions (V)4″[1]
Notable featuresBipolar outflow, Bipolar nebula
DesignationsPN M 2-42

PNG 008.2-04.8
PK 008-04 2
Hen 2-393
ESO 522-21
PN Sa 2-331

WRAY 16-409
See also: Lists of nebulae

Minkowski 2-42, abbreviated M2-42, is a planetary nebula that was discovered by Rudolph Minkowski in 1947.[2] It is located about 30,800 light-years away from Earth in the Galactic bulge.[1] It is known to be a bipolar planetary nebula containing two jets of material emerging from both sides of its central star.[3] It has been found that its bipolar outflows have the typical features of Fast Low-Ionization Emission Region (FLIER). [3]

The central star of M2-42 is classified as weak emission-line star,[4] but its nitrogen and helium features[5] may be linked to nitrogen sequences of Wolf-Rayet central stars of planetary nebula ([WN]).[3] The chemical composition of this planetary nebula was found to be around the solar metallicity.[6]

Image of M2-42 taken by the VLT Survey Telescope. The green part of the image was taken with a H-alpha filter.

See also

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 "PN M2-42". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=PN+M2-42. 
  2. ↑ Minkowski, R. (1947). "New Emission Nebulae (II)". Publications of the Astronomical Society of the Pacific 59 (350): 257. doi:10.1086/125962. Bibcode: 1947PASP...59..257M. 
  3. ↑ 3.0 3.1 3.2 Danehkar, A.; Parker, Q. A.; Steffen, W. (2016). "Fast, low-ionization emission regions of the planetary nebula M2-42". The Astrophysical Journal 151 (2): 38. doi:10.3847/0004-6256/151/2/38. Bibcode: 2016AJ....151...38D. 
  4. ↑ Tylenda, R.; Acker, A.; Stenholm, B. (1993). "Wolf-Rayet nuclei of planetary nebulae. Observations and classification". Astronomy and Astrophysics Supplement Series 102: 595–602. Bibcode: 1993A&AS..102..595T. 
  5. ↑ DePew, K.; Parker, Q. A.; Miszalski, B.; De Marco, O.; Frew, D. J.; Acker, A.; Kovacevic, A. V.; Sharp, R. G. (2011). "Newly discovered Wolf-Rayet and weak emission-line central stars of planetary nebulae". Monthly Notices of the Royal Astronomical Society 414 (4): 2812–2827. doi:10.1111/j.1365-2966.2011.18337.x. Bibcode: 2011MNRAS.414.2812D. 
  6. ↑ Wang, W.; Liu, X. -W. (2007). "Elemental abundances of Galactic bulge planetary nebulae from optical recombination lines". Monthly Notices of the Royal Astronomical Society 381 (4): 669–701. doi:10.1111/j.1365-2966.2007.12198.x. Bibcode: 2007MNRAS.381..669W. 

Coordinates: Sky map 18h 22m 32.08s, −24° 09′ 27.7″




Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:M2-42&oldid=3354105"