
NGC 2547 - Wikipedia
NGC 2547 is a southern open cluster in Vela, discovered by Nicolas Louis de Lacaille in 1751 [2] [3] from South Africa. The star cluster is young with an age of 20-30 million years. [4] …
NGC 2547 - 维基百科,自由的百科全书
NGC 2547 是一個位於南半球天空的 疏散星團,位於 船帆座。 該星團由法國天文學家 尼可拉·路易·拉卡伊 於1751至1752年間在南非發現。 該星團的角直徑約20',視星等4.7等。 年齡只 …
NGC 2547 - Open Cluster in Vela | TheSkyLive.com
NGC 2547 is a Open Cluster in the Vela constellation. NGC 2547 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual …
NGC 2547 - 維基百科,自由的百科全書 - zh.wikipedia.org
NGC 2547 是一個位於南半球天空的 疏散星團,位於 船帆座。 該星團由法國天文學家 尼可拉·路易·拉卡伊 於1751至1752年間在南非發現。 該星團的角直徑約20',視星等4.7等。 年齡只 …
Young, hot, and blue: stars in cluster NGC 2547
2013年3月27日 · While NGC 2547 contains many hot stars that glow bright blue, a telltale sign of their youth, you can also find one or two yellow or red stars, which have already evolved to …
2MASS J08090250-4858172 - Wikipedia
2MASS J08090250-4858172 (also called NGC 2547–ID8) is a star in the cluster NGC 2547. In 2014 it was reported that the star had brightened in the infrared. This was interpreted as a …
NGC2547 (Open cluster) - In-The-Sky.org
R/B-band color composite image from the Second Digitized Sky Survey (DSS2), measuring 10 arcminutes across. Click and drag the chart above to pan around the sky, or use the mouse …
NGC 2547 open cluster, RGB - AstroBin
NGC 2547 is a large (20') and super bright (4.7 Mag) open cluster in the constellation Vela. NGC 2547 was formed about 30 million years ago. NGC 2547 contains many stars with debris …
Stars of the cluster NGC 2547 | Science Wire - EarthSky
2013年3月27日 · The star cluster NGC 2547 lies in the southern constellation of Vela (The Sail), about 1500 light-years from Earth, and is bright enough to be easily seen using binoculars.
Spitzer Observations of NGC 2547: The Disk Population at 25 …
2004年9月1日 · We present Spitzer observations of the young cluster NGC 2547, obtaining photometry at 3.6, 4.5, 5.8, 8.0, and 24 μm, reaching significantly fainter infrared sensitivities …