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.

NGC 588 是 三角座 的一個 星系。 它是由德国-丹麦天文学家 海因里希·路易·达雷 於1861年10月2日发现。 它的赤經為1時32分45.7秒，赤緯為30°38'56"，星等為13.5 [1][2][3]。 ^ Rojas, Sebastián García. Diffuse nebula NGC 588 · Deep Sky Objects Browser. DSO Browser. [2017-05-12]. （原始内容 存档于2018-01-01） （英语）. ^ NGC 588. simbad.u-strasbg.fr. [2017-05-14]. （原始内容 存档于2018-01-01）.

2011年1月10日 · Download a PDF of the paper titled A 2D multiwavelength study of the ionized gas and stellar population in the Giant HII Region NGC 588, by A. Monreal-Ibero (1 and 11 other authors

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.

NGC 588 is a Diffuse Nebula located in the constellation of Triangulum in the northern hemisphere. NGC 588 is called NGC 588 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work.

We present the results of a double analysis of the ionizing cluster in NGC 588, a giant HII region (GHR) in the outskirts of the nearby galaxy M 33. For this purpose, we obtained ground based long-slit spectroscopy and combined it with archival ground based and space borne imaging and spectroscopy, in the wavelength range 1100-9800 Å.

From Virginia Beach , NGC588 is not observable – it will reach its highest point in the sky during daytime and is no higher than 21° above the horizon at dusk.

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.

1992年4月30日 · The peculiar giant extragalactic HII region NGC 588 has been observed with the TAURUS Fabry-Perot Spectrograph at the William Hershell Telescope of the Observatorio del Roque de los Muchachos....

2005年9月20日 · 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...