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Long-term monitoring of active stars. VIII. UBV(RI)_(c) photometry collected in February 1992
As a part of an extensive program focusing on the global properties andevolution of active stars, high-precision UBV(RI)_c photometry of 31selected stars, collected at the European Southern Observatory over the14-29 February 1992 interval, is presented. Significant evolution of thelight curves, period variations and evidence for long-term variabilityof the global degree of spottedness are found. Some spectralclassifications are revised and the inferred photometric parallaxes arecompared, whenever possible, with the values measured by the Hipparcossatellite. Flare events were detected for the star HD16157 = CC Eri, EXO 055609-3804.4 TY Coland HD 119285 = V851 Cen. Optical variability wasdiscovered for the Pop II binary HD 89499. Theseobservations contribute to the establishment of a time-extendedphotometric database which can give important clues on topics such asthe stability of spotted areas, differential rotation, solar-like cyclesand the correlation between inhomogeneities at different atmosphericlevels. based on data collected at the European Southern Observatory, LaSilla, Chile.
| Photometric and spectroscopic studies of cool stars discovered in EXOSAT X-ray images. I - Time variability and spectral classification of eight southern stars
As part of a larger program to study the optical properties ofserendipitous Exosat sources, optical photometry and low-resolutionspectroscopy are presented for eight southern stars which have beenidentified as optical counterparts of Exosat sources. X-ray fluxvariability has been detected for three of them. In all three cases theoptical counterparts show RS CVn-type variability. Of the remaining fivestars, two are found to be variable in the optical. The high X-rayluminosities inferred from the derived spectroscopic parallaxesindicates that these variable sources are all very active systems,possibly RS CVn binaries. The three nonvariable sources are more likelynormal main-sequences stars, two of them with a rather high level ofcoronal emission.
| Einstein Observatory magnitude-limited X-ray survey of late-type giant and supergiant stars
Results are presented of an extensive X-ray survey of 380 giant andsupergiant stars of spectral types from F to M, carried out with theEinstein Observatory. It was found that the observed F giants orsubgiants (slightly evolved stars with a mass M less than about 2 solarmasses) are X-ray emitters at the same level of main-sequence stars ofsimilar spectral type. The G giants show a range of emissions more than3 orders of magnitude wide; some single G giants exist with X-rayluminosities comparable to RS CVn systems, while some nearby large Ggiants have upper limits on the X-ray emission below typical solarvalues. The K giants have an observed X-ray emission level significantlylower than F and F giants. None of the 29 M giants were detected, exceptfor one spectroscopic binary.
| Walraven photometry of nearby southern OB associations
Homogeneous Walraven (VBLUW) photometry is presented for 5260 stars inthe regions of five nearby southern OB associations: Scorpio Centaurus(Sco OB2), Orion OB1, Canis Major OB1, Monoceros OB1, and Scutum OB2.Derived V and (B - V) in the Johnson system are included.
| Studies of calcium emission stars - I. HD 158393 a giant star in a binary system.
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| Radial velocities of southern stars obtained with the photoelectric scanner CORAVEL. III - 790 late-type bright stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1985A&AS...59...15A&db_key=AST
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Osservazione e dati astrometrici
| Costellazione: | Scorpione |
| Ascensione retta: | 17h31m47.40s |
| Declinazione: | -33°42'10.0" |
| Magnitudine apparente: | 6.44 |
| Distanza: | 123.001 parsec |
| Moto proprio RA: | -7.9 |
| Moto proprio Dec: | -31.3 |
| B-T magnitude: | 7.965 |
| V-T magnitude: | 6.548 |
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