dc.contributor.author |
Bappu, M. K. V |
|
dc.date.accessioned |
2007-11-28T10:19:53Z |
|
dc.date.available |
2007-11-28T10:19:53Z |
|
dc.date.issued |
1954 |
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dc.identifier.citation |
Monthly Notices of Royal Astronomical Society, Vol. 114, No. 6, pp. 687-691 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/1981 |
|
dc.description.abstract |
Photoelectric colours and magnitudes have been determined for twenty-five stars considered to be members of the moving cluster in Perseus. A distance modulus of 6m.83, corresponding to a distance of 230 ps, has been derived. This value is nearly twice the value of 120 ps derived by Miss Roman and Morgan from the upsilon component of proper motion. |
en |
dc.format.extent |
344049 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Royal Astronomical Society |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1954MNRAS.114..687V |
en |
dc.subject |
Photoelectric Colours and Magnitudes |
en |
dc.subject |
Perseus Cluster |
en |
dc.subject |
M.K.V. Bappu |
en |
dc.title |
Magnitudes and colours of some members of the Perseus Cluster |
en |
dc.type |
Article |
en |