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  1. NGC 588 - Wikipedia

    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.

  2. NGC 588 - HII Ionized region in Triangulum | TheSkyLive.com

    NGC 588 is a HII Ionized region in the Triangulum constellation. NGC 588 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its visual magnitude of 14.44, NGC 588 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

  3. Some of M33's HII regions - Sketching - Cloudy Nights

    Nov 10, 2023 · NGC 588 was the last of these seen, further out than 592 but much fainter. It was first spotted in AV and was quite persistent as a faint smudge. 595 and 592 could be held in direct vision once I knew where they were.

  4. NGC 588 - Wikiwand

    NGC 588 is a prominent, giant H II ionized diffuse nebula located in the outskirts of the galaxy Messier 33's spiral arms, within the Triangulum constellation. 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.

  5. On the importance of the few most massive stars: The ionizing cluster ...

    We discuss the results in terms of the strong influence of the few most massive stars, six in the case of NGC 588, that dominate the overall SED and, in particular, the ionizing far ultraviolet range beyond the Lyman limit.

  6. What is the temperature structure in the giant HII region NGC 588?

    Sep 20, 2005 · We present the results of an exhaustive study of the ionized gas in NGC 588, a giant H II region in the nearby spiral galaxy M33. This analysis uses a high number of diagnostics in the optical and infrared ranges.

  7. [1101.1853] A 2D multiwavelength study of the ionized gas and …

    Jan 10, 2011 · (ABRIDGED) We present an analysis of NGC588 based on IFS data with PMAS, together with Spitzer images at 8 mi and 24 mi. The extinction distribution in the optical shows complex structure, with maxima correlating in position with those of the emission at …

  8. NGC 588 — Wikipédia

    NGC 588 est une nébuleuse en émission renfermant un amas ouvert. Cette nébuleuse est une région HII de la galaxie du Triangle (M33). Elle est donc située dans la constellation du Triangle. NGC 588 a été découverte par l'astronome prussien Heinrich d'Arrest en 1861.

  9. NGC 588 - Nebula - WIKISKY

    What is the temperature structure in the giant HII region NGC 588? We present the results of an exhaustive study of the ionized gas inNGC 588, a giant Hii region in the nearby spiralgalaxy M 33. This analysis uses a high number ofdiagnostics in the optical and infrared ranges.

  10. NGC 588 | H II region in Triangulum | New General Catalogue

    < NGC List NGC 588. NGC 588 is a H II region located in the constellation of Triangulum. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 588:

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