dc.contributor.author |
Cannon, R. D |
|
dc.contributor.author |
Sagar, R |
|
dc.contributor.author |
Hawkins, M. R. S |
|
dc.date.accessioned |
2008-09-16T14:09:23Z |
|
dc.date.available |
2008-09-16T14:09:23Z |
|
dc.date.issued |
1990-03 |
|
dc.identifier.citation |
Monthly Notices of Royal Astronomical Society, Vol. 243, No. 1, pp. 151 - 158 |
en |
dc.identifier.issn |
0035-8711 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3643 |
|
dc.description.abstract |
A V, (B-V) C-M diagram for the distant globular cluster NGC 5824 is obtained from CCD observations of 285 stars reaching V = 20.5. Assuming a reddening of E(B-V) = 0.13, the color of the giant branch at the level of the horizontal branch is found to be (B-V)o,g = 0.77, while the apparent distance modulus (V-Mv) is shown to be 18.0 + or - 0.2. Also, an Fe/H abundance ratio = -1.7 and a heliocentric distance of 33 + or - 3 kpc are estimated. The results produce a galactocentric distance of 25 kpc. This result is combined with the radial-velocity determination of Hesser, Shawl, and Meyer (1986), making it possible to plot the representative point of the cluster in Lynden and Bell's (1983) velocity-distance diagram. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Royal Astronomical Society |
en |
dc.relation.uri |
http://ads.iucaa.ernet.in/abs/1990MNRAS.243..151C |
en |
dc.subject |
Astronomical photometry |
en |
dc.subject |
Charge coupled devices |
en |
dc.subject |
Color-magnitude diagram |
en |
dc.subject |
Globular clusters |
en |
dc.subject |
Galactic mass |
en |
dc.subject |
Interstellar extinction |
en |
dc.subject |
Metallicity |
en |
dc.subject |
Milky Way galaxy |
en |
dc.subject |
Southern sky |
en |
dc.title |
CCD photometry of the distant southern globular cluster NGC 5824 |
en |
dc.type |
Article |
en |