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Broad-band photometry of selected southern ultraviolet-bright stars.
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| A survey of ultraviolet objects
An all-sky survey of ultraviolet objects is presented together with astatistical analysis that leads to the conclusion that there is asignificantly higher population of hot subdwarfs lying below themain-sequence than hitherto thought. The distribution of all ultravioletobjects, main sequence ultraviolet objects, and MK unclassifiedultraviolet objects are shown in galactic coordinates, and the absolutemagnitudes and color-color diagrams for these groups are presented.Scale heights are derived, giving values similar to planetary nebulaefor the hottest groups.
| Ultraviolet spectrophotometry of a group of hot stars in Vela
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| Behavior of lambda 2800 Mg II in stellar spectra
The results of measurements of the equivalent widths of the resonancedoublet of ionized magnesium lambda 2800 Mg II in the spectra of 51relatively faint stars, up to 10m, of the spectral classes B1-K5 arepresented. The observed material has been obtained by means of the spaceobservatory 'Orion 2'. Some regularities in the behavior of lambda 2800Mg II in stellar spectra have been revealed: wide and deep depression ofthe continuous spectra at 2800 A in F-G type stars; the presence of thedoublet lambda 2800 Mg II in the form of weak emission in the spectra ofcold stars (K2-K5); the presence both of the multiplet lambda 3080 Ti IIand the doublet lambda 2800 Mg II simultaneously either in emission - inthe late-type stars - or in absorption in earlier types; the existenceof combined profiles of lambda 2800 Mg II, i.e., a wide absorption linewith a weak emission in the center, in stars of the transitional class(G5-K0), etc. A well-defined empirical relationship between theequivalent width of lambda 2800 Mg II and the spectral class of the starhas been established.
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| Takýmyýldýz: | Yelken |
| Sað Açýklýk: | 09h17m59.73s |
| Yükselim: | -45°38'10.6" |
| Görünürdeki Parlaklýk: | 7.182 |
| Uzaklýk: | 454.545 parsek |
| özdevim Sað Açýklýk: | -6.8 |
| özdevim Yükselim: | 1.3 |
| B-T magnitude: | 7.018 |
| V-T magnitude: | 7.169 |
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