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・ NGC 80
・ NGC 800
・ NGC 81
・ NGC 82
・ NGC 83
・ NGC 6357
・ NGC 6362
・ NGC 6366
・ NGC 637
・ NGC 6380
・ NGC 6384
・ NGC 6388
・ NGC 6397
・ NGC 64
・ NGC 6401
NGC 6496
・ NGC 65
・ NGC 6503
・ NGC 6520
・ NGC 6522
・ NGC 6530
・ NGC 6539
・ NGC 6541
・ NGC 6559
・ NGC 6560
・ NGC 6565
・ NGC 6566
・ NGC 6570
・ NGC 6572
・ NGC 6578


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NGC 6496 : ウィキペディア英語版
NGC 6496

NGC 6496 is a globular cluster which is in the direction of the bulge and putative members of this subgroup, based on observations collected with the WFPC2 on board the Hubble Space Telescope. NGC 6496 was originally believed to be a member of the disc system of GC, but scientists questioned this classification. It was instead suggested that NGC 6496, together with two other clusters, NGC 6624 and NGC 6637, could be halo clusters with strongly inclined orbits. NGC 6496 lies in the Southern sky at RA=17:59:03.68 and Dec=-44:15:57.4.
The first CMD presented of NGC 6496 had photometry reaching 2 mag below the horizontal branch, disclosing for the first time the usual red arm of the metal-rich clusters. The extinction towards NGC 6496 is uncertain, with estimates ranging between E(B-V) = 0.09 and E(B-V) = 0.24.
== References ==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「NGC 6496」の詳細全文を読む



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