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Observed Orbital Eccentricities
For 391 spectroscopic and visual binaries with known orbital elementsand having B0-F0 IV or V primaries, we collected the derivedeccentricities. As has been found by others, those binaries with periodsof a few days have been circularized. However, those with periods up toabout 1000 or more days show reduced eccentricities that asymptoticallyapproach a mean value of 0.5 for the longest periods. For those binarieswith periods greater than 1000 days their distribution of eccentricitiesis flat from 0 to nearly 1, indicating that in the formation of binariesthere is no preferential eccentricity. The binaries with intermediateperiods (10-100 days) lack highly eccentric orbits.
| Statistics of spectroscopic sub-systems in visual multiple stars
A large sample of visual multiples of spectral types F5-M has beensurveyed for the presence of spectroscopic sub-systems. Some 4200 radialvelocities of 574 components were measured in 1994-2000 with thecorrelation radial velocity meter. A total of 46 new spectroscopicorbits were computed for this sample. Physical relations are establishedfor most of the visual systems and several optical components areidentified as well. The period distribution of sub-systems has a maximumat periods from 2 to 7 days, likely explained by a combination of tidaldissipation with triple-star dynamics. The fraction of spectroscopicsub-systems among the dwarf components of close visual binaries withknown orbits is similar to that of field dwarfs, from 11% to 18% percomponent. Sub-systems are more frequent among the components of widevisual binaries and among wide tertiary components to the known visualor spectroscopic binaries - 20% and 30%, respectively. In triple systemswith both outer (visual) and inner (spectroscopic) orbits known, we findan anti-correlation between the periods of inner sub-systems and theeccentricities of outer orbits which must be related to dynamicalstability constraints. Tables 1, 2, and 6 are only available inelectronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr(130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/382/118
| Infrared Speckle Interferometry of Eleven Binaries Using a Bispectral Analysis
Infrared speckle-masking observations of eleven binary systems with the6-m Special Astrophysical Observatory telescope are presented. Aresolution of 43 mas in J (1.25 micrometer) and 76 mas in K (2.2micrometers) has been achieved in reconstructed images. Accuratemagnitude differences, separations, and position angles have beendetermined for all the resolved binaries. The pair HR 1071 with anabnormally low lithium abundance is considered in more detail.
| New spectroscopic components in multiple systems. IV.
New close sub-systems are reported and studied in eight visual multiplesystems. Elements of one double-lined and eight single-linedspectroscopic orbits are given. Magnitudes, colors, spectral types andmasses of individual components are estimated by combining all availabledata. The visual secondary component of the young binary HD 27638 is adouble-lined pair of G-type dwarfs on a 17-day orbit with an unseen butmassive (>1.2 Msun) spectroscopic tertiary on an 8-yearorbit. The invisible secondary of HD 28271A is also massive, but it isnot seen, probably because of a high luminosity of the primary - an F7star with fast axial rotation and an active chromosphere which evolvesoff the Main Sequence. Two additional companions are found in the visualtriple system HD 179484. Table 4 is only available in electronic form atthe CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5)} or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/374/227
| The Henry Draper Extension Charts: A catalogue of accurate positions, proper motions, magnitudes and spectral types of 86933 stars
The Henry Draper Extension Charts (HDEC), published in the form offinding charts, provide spectral classification for some 87000 starsmostly between 10th and 11th magnitude. This data, being highlyvaluable, as yet was practically unusable for modern computer-basedastronomy. An earlier pilot project (Roeser et al. 1991) demonstrated apossibility to convert this into a star catalogue, using measurements ofcartesian coordinates of stars on the charts and positions of theAstrographic Catalogue (AC) for subsequent identification. We presenthere a final HDEC catalogue comprising accurate positions, propermotions, magnitudes and spectral classes for 86933 stars of the HenryDraper Extension Charts.
| Erreurs relevées dans le Catalogue Index 1961. 0
Not Available
| Binary star speckle measurements during 1989-1993 from the SAO 6 M and 1 M telescopes in Zelenchuk
We have continued to survey visual and interferometric binary stars withsignificant orbital motion by means of speckle method at the telescopesof the Special Astrophysical Observatory (SAO) in Zelenchuk. Here wepresent the lists of 267 speckle observations made with the 6 m and the1 m telescopes in the period May 1989-November 1993.
| The chromospheric emission-age relation for stars of the lower main sequence and its implications for the star formation rate
An attempt is made to formulate the relationship between age andchromospheric emission (CE) in late-type dwarf stars. Evidence isreviewed that a deterministic relationship of this type actually exists,and that for stars of known age, either a power-law relation or a curvecorresponding to a constant star formation rate fits equally well.Further observations should be able to demonstrate either that there isa real excess of young stars near the sun or that the evolution of CEfor a low-mass star goes through a slow initial decline, a rapid declineat intermediate ages, and finally a slow decline for old stars like thesun.
| Absolute far-ultraviolet spectrophotometry of hot subluminous stars from Voyager
Observations, obtained with the Voyager ultraviolet spectrometers, arepresented of absolute fluxes for two well-known hot subluminous stars:BD + 28 deg 4211, an sdO, and G191 - B2B, a hot DA white dwarf. Completeabsolute energy distributions for these two stars, from the Lyman limitat 912 A to 1 micron, are given. For BD + 28 deg 4211, a single powerlaw closely represents the entire observed energy distribution. For G191- B2B, a pure hydrogen model atmosphere provides an excellent match tothe entire absolute energy distribution. Voyager absolute fluxes arediscussed in relation to those reported from various sounding rocketexperiments, including a recent rocket observation of BD + 28 deg 4211.
| UVBY photometry of wide visual double stars with B, A and F spectral type- I.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1978A&AS...34..453O&db_key=AST
| Rotational velocities and spectral types for a sample of binary systems.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1975A&AS...19...91L&db_key=AST
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Observation and Astrometry data
| Constellation: | おうし座 |
| Right ascension: | 04h35m35.18s |
| Declination: | +10°10'13.6" |
| Apparent magnitude: | 7.785 |
| Proper motion RA: | 51.8 |
| Proper motion Dec: | -49.4 |
| B-T magnitude: | 8.431 |
| V-T magnitude: | 7.839 |
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