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 是三角座的一个星系。 它是由德国-丹麦天文学家 海因里希·路易·达雷 于1861年10月2日发现。 它的赤经为1时32分45.7秒，赤纬为30°38'56"，星等为13.5 [ 1 ] [ 2 ] [ 3 ] 。

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, …

6 天之前 · NGC 588 (NGC588) is a diffuse nebula that has a distance from Earth of light years. It can be found in the constellation of Triangulum.

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

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...

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.

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.

We present a detailed multiwavelength photometric study of giant H II regions NGC 592 and NGC 588 in the nearby small spiral galaxy M33. We use data taken with the Wide Field and Planetary Camera 2 (WFPC2) on board the Hubble Space Telescope (HST).

2024年5月22日 · NGC 588 是 三角座 的一个 星系。 它是由德国-丹麦天文学家 海因里希·路易·达雷 于1861年10月2日发现。 它的赤经为1时32分45.7秒，赤纬为30°38'56"，星等为13.5 …