| 词条 | NGC 5927 |
| 释义 |
| name = NGC 5927 | class = VIII | image = | caption = The globular cluster NGC 5927 | credit = HST | epoch = J2000 | constellation = Lupus | ra = {{RA|15|28|00.69}}[1] | dec = {{DEC|-50|40|22.9}}[1] | dist_ly = 25.1 kly (7.7 kpc)[1] | appmag_v = 8.86[1] | size_v = | mass_msol = | radius_arcminsec = 6.0' x 6.0'[2] | v_hb = | metal_fe = -0.49[3] | metal_z = | age = | notes = | names = GCl 35, GCRV 5278 E, VDBH 173[1] }} NGC 5927 is a globular cluster in the constellation Lupus. NGC 5927 has a diameter of about 12 arcminutes and an apparent magnitude of +8.86. Its Shapley–Sawyer Concentration Class is VIII,[2] and it contains stars of magnitude 15 and dimmer. The globular cluster was discovered by the astronomer James Dunlop in 1826 with a 9-inch telescope and later by John Louis Emil Dreyer in the New General Catalog.[2] References1. ^1 2 3 4 {{cite simbad|title=NGC 5927|accessdate=8 January 2017}} 2. ^1 2 {{cite web|title=NGC 5927|url=http://spider.seds.org/spider/MWGC/n5927.html|accessdate=8 January 2016}} 3. ^{{cite web|title=A Galactic Globular Clusters Database: NGC 5927|url=http://gclusters.altervista.org/cluster_4.php?ggc=NGC+5927|accessdate=8 January 2017}} External links
3 : Globular clusters|Lupus (constellation)|NGC objects |
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