Diffuse nebula | |
---|---|
Observation data: epoch | |
Subtype | H II[1] |
Right ascension | 1h 32.7m 00s[2] |
Declination | +30° 40′ 00″[2] |
Distance | z=-0.000580[1] |
Apparent dimensions (V) | 0.65 arc minutes?[3] |
Constellation | Triangulum |
Designations | IRAS 01299+3023[4] |
NGC 588 is a prominent, giant H II ionized[5] diffuse nebula located in the outskirts of the galaxy Messier 33's spiral arms, within the Triangulum constellation.[6][4] The nebula has two Wolf-Rayet stars, NGC 588-UIT 008 and NGC 588-MC3 and a fairly large population of main sequence stars of 2 to 20 solar masses. The more massive stars in the nebula have a mass of around 40 solar masses. NGC 588 is 4.2 million years old and has a mass of 2300 solar masses.[7]
NGC 588 and NGC 592 (another nebula in the Triangulum galaxy) are both very prominent stellar nurseries in their regions.[8]
Discovery
It was discovered October 2, 1861 by the German-Danish astronomer Heinrich d'Arrest.[9]
References
- 1 2 "NGC 588". ned.ipac.caltech.edu.
- 1 2 "Ngc 588".
- ↑ "New General Catalog Objects: NGC 550 - 599".
- 1 2 "NGC 588". simbad.u-strasbg.fr. Retrieved 2017-05-14.
- ↑ "NGC 588 - HII Ionized region in Triangulum | TheSkyLive.com". theskylive.com. Retrieved 2023-10-26.
- ↑ Rojas, Sebastián García. "Diffuse nebula NGC 588 · Deep Sky Objects Browser". DSO Browser. Archived from the original on 2018-01-01. Retrieved 2017-05-12.
- ↑ academic.oup.com https://academic.oup.com/mnras/article/394/4/1847/1200418. Retrieved 2023-10-26.
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(help) - ↑ https://academic.oup.com/mnras/article/394/4/1847/1200418. Retrieved 2023-10-26.
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(help) - ↑ "New General Catalog Objects: NGC 550 - 599". cseligman.com. Retrieved 2017-05-12.
External links
- Media related to NGC 588 at Wikimedia Commons
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