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Query : 2006A&A...449..161D |
2006A&A...449..161D - Astronomy and Astrophysics, volume 449, 161-170 (2006/4-1)
Why is the mass function of NGC 6218 flat?
DE MARCHI G., PULONE L. and PARESCE F.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): stars: Hertzsprung-Russell (HR) and C-M diagrams - stars: luminosity function, mass function - globular clusters: general - Galaxy: globular clusters: individual: NGC6218
Simbad objects: 6
Number of rows : 6 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | NGC 104 | GlC | 00 24 05.359 | -72 04 53.20 | 4.09 | ~ | 3917 | 0 | ||||
2 | NAME Serpens Dwarf | GlC | 15 16 05.30 | -00 06 41.0 | 15.1 | ~ | 734 | 1 | ||||
3 | M 12 | GlC | 16 47 14.18 | -01 56 54.7 | 6.07 | ~ | 677 | 0 | ||||
4 | NGC 6397 | GlC | 17 40 42.09 | -53 40 27.6 | 5.17 | ~ | 1976 | 0 | ||||
5 | NGC 6712 | GlC | 18 53 04.32 | -08 42 21.5 | ~ | 519 | 0 | |||||
6 | M 15 | GlC | 21 29 58.33 | +12 10 01.2 | ~ | 3140 | 0 |
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