NGC 2359

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Emission nebula
NGC 2359 / Duck Nebula

Image taken with the 81 cm reflecting telescope of the Mount Lemmon Observatory

Image taken with the 81 cm reflecting telescope of the Mount Lemmon Observatory
AladinLite
Constellation Big dog
Position
equinoxJ2000.0 , epoch : J2000.0
Right ascension 07 h 18 m 31.0 s
declination -13 ° 13 ′ 38 ″
Appearance

Apparent brightness  (visual) +11.45 mag  
Angular expansion 9 ′ × 6 ′ 
Ionizing source
designation HD 56925 (WR 7, HIP 35378) 
Type WN 
Physical data

Affiliation Milky Way 
distance  approx. 15000 ly
(approx. 5000 pc )
history

discovery Wilhelm Herschel
Date of discovery January 31, 1785
Catalog names
 NGC  2359 • LBN 1041, Sh2-298, Gum 4, RCW  5, GC 1511, h 3075, H V 21

NGC 2359 , also known as the Duck Nebula and Thor's Helmet , is a Wolf-Rayet Ring Nebula (a special type of emission nebula ) in the constellation Great Dog . NGC 2359 has an apparent magnitude of +11.45 mag and an angular extent of 9 ′ × 6 ′. It is about 15,000 light years away from the solar system and has a diameter of about 20 light years . It expands at 26 kilometers per second. The mass of the bubble is estimated to be 70 to 140 solar masses .

In contrast to most of the others, this emission nebula is not excited to glow by O stars (such as the Orion Nebula ) or white dwarfs (such as the planetary nebulae ), but by a Wolf-Rayet star : HD 56925 (WR 7 , HIP 35378). This 11.4 mag bright star is located a little west of the center of the bubble and has an effective temperature of approx. 50,000 ° Celsius. The star builds up enormous radiation pressure , which blows the outer shells into interstellar space . The matter expelled and expelled over time forms a bubble which marks the front of the ejection.

Spectral analyzes suggest that the bubble-shaped nebula presumably consists of a mixture of material that the central Wolf-Rayet star lost in an earlier ejection and of the surrounding interstellar medium , which swirls, condenses and through the interaction with its strong stellar wind is ionized.

The object was discovered on January 31, 1785 by William Herschel . The object was cataloged by Wilhelm Tempel in 1877 as NGC 2361 , which describes part of the nebula.

Web links

Commons : NGC 2359  - album containing pictures, videos and audio files

Individual evidence

  1. NASA / IPAC EXTRAGALACTIC DATABASE
  2. SEDS : NGC 2359
  3. Michael Fritz in: Stars and Space February 2015 p. 60f
  4. ^ Adrian Kaminski in: Stars and Space December 2014 p. 14
  5. Seligman