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Long-term monitoring of active stars. IX. Photometry collected in 1993
As a part of an extensive program focused on the global properties andevolution of active stars, high-precision UBV(RI)_c and UBV photometryof 31 selected stars is presented. The UBV(RI)_c observations werecollected at the European Southern Observatory over the 31 December1992-18 January 1993 and the 20 November-3 December 1993 intervals.Additional UBV photometry obtained by the ``Phoenix" and by the CataniaAstrophysical Observatory Automatic Photoelectric Telescopes from 1990to 1993 is also presented for some of the program stars. Significantevolution of the light curves, period variations and evidence forlong-term variability of the global degree of spottedness are found.Some spectral classifications are revised and the inferred photometricparallaxes are compared, whenever possible, with the values measured bythe Hipparcos satellite. These observations are finalized to theconstruction of an extended photometric database, which can giveimportant clues on topics such as the stability of spotted areas,differential rotation, solar-like cycles and the correlation betweeninhomogeneities at different atmospheric levels. Based on data collectedat the European Southern Observatory, La Silla, Chile. Tables and thecomplete data set are also available in electronic form at the CDS viaanonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/367/910
| Photometric and spectroscopic studies of cool stars discovered in EXOSAT X-ray images. III. Photometric properties.
We present high-precision UBV(RI)_c_ photometry for a sample of activestars detected serendipitously by the EXOSAT satellite. Fourteenobjects, out of 47 likely optical counterparts, turned out to be clearlyvariable, with periods in the range 1-8 days, including a newlydiscovered eclipsing binary. For most of them the optical variability isconsistent with the presence of photospheric cool spots. We have usedour multicolour photometry to estimate spectral classifications anddistances. The derived distances indicate that some of the observedstars are previously unidentified nearby (d<=25pc) M dwarfs. Whencombined with the results of high resolution spectroscopy, ourphotometric observations allow us to investigate the stellar content ofthe selected X-ray sample. Young stars and RS CVn-type binaries appearto constitute a large fraction of the selected sample.
| The EXOSAT high Galactic latitude survey
This study presents a survey of serendipitous sources performed in thevery soft X-ray band (0.05-2.0 keV) using the Exosat imaging telescopes.It covers 783 sq deg of high Galactic latitude sky and includes 210serendipitous sources which define a complete (flux-limited) sample. Twohundred of the 210 detected sources are identified via extensive opticaland radio observations together with cross-correlations with catalogs ofknown objects. The log N-log S relation was found to be consistent withthat of the Einstein extended Medium-Sensitivity Survey (EMSS) and withthe 'Euclidean' value of 1.5. The normalization of the relation is astrong function of the assumed spectral slope of AGN. It is inferredfrom the consistency with the EMSS results that the average (energy)slope of extragalactic sources in the soft X-ray band is very steep(approximately 1.5). An analysis of the association between AGNdetection and Galactic N(H) also shows that the average slope is steepand inconsistent with the canonical value of 0.7.
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Tavus |
| Sað Açýklýk: | 18h32m53.00s |
| Yükselim: | -65°15'41.7" |
| Görünürdeki Parlaklýk: | 7.807 |
| Uzaklýk: | 591.716 parsek |
| özdevim Sað Açýklýk: | 7.3 |
| özdevim Yükselim: | -15.4 |
| B-T magnitude: | 7.774 |
| V-T magnitude: | 7.805 |
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