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CCD photometry and astrometry of visual double and multiple stars of the HIPPARCOS Catalogue. II. CCD photometry and differential astrometry of 288 southern ``Intermediate'' systems
We present photometric and astrometric data of about 280 visual doublestars of the ``intermediate'' class, i.e. with angular separationsmainly in the range 2arcsec < rho < 12arcsec . The observationshave been obtained in 1991-92 with a CCD camera attached to the 91 cmDutch telescope at ESO La Silla, Chile. Differential magnitudes of thedouble star components as well as magnitudes and colour indices of theindividual components have been determined in the Cousins V and Ipassbands with an internal error of about 0.005 mag and an externalaccuracy of less than 0.03 mag. In addition, angular separations havebeen secured to an internal accuracy of 0.004arcsec and position anglesto about 0.05degr. Tables 1 to 4 are only available in electronic format the CDS via ftp to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/Abstract.html. Based on observationscollected at the European Southern Observatory, La Silla, Chile.
| Far-ultraviolet stellar photometry: A field in Orion
Far-ultraviolet photometry for 625 objects in Orion is presented. Thesedata were extracted from electrographic camera images obtained duringsounding rocket flights in 1975 and 1982. The 1975 images were centeredclose to the belt of Orion while the 1982 images were centeredapproximately 9 deg further north. One hundred and fifty stars fell inthe overlapping region and were observed with both cameras. Sixty-eightpercent of the objects were tentatively identified with known starsusing the SIMBAD database while another 24% are blends of objects tooclose together to separate with our resolution. As in previous studies,the majority of the identified ultraviolet sources are early-type stars.However, there are a significant number for which no such identificationwas possible, and we suggest that these are interesting objects whichshould be further investigated. Seven stars were found which were brightin the ultraviolet but faint in the visible. We suggest that some ofthese are nearby white dwarfs.
| Spectroscopic binaries in the Orion OB1 association
A radial velocity study of the brighter members of the Ori OB2association is reported. The radial velocity variables, new preliminaryorbital elements for six spectroscopic binaries, and the projected axialrotation in stars for which the orbital elements are lacking arereported. The correlation between the proportion of binaries and theaverage axial rotation for the subgroups of the association isdiscussed. It is found that the Orion main-sequence members rotate atalmost the same rate as field stars of the same types. The averageradial velocity for the whole association is 23 km/s. The percentage ofspectroscopic binaries with periods shorter than 100 days plus themagnetic Ap-Bp among the main-sequence members of the association is 32percent.
| Studies of the local interstellar medium. VIII - Morphology and kinematics of the diffuse interstellar clouds toward Orion
Interstellar clouds in the direction of the Orion association show onlypositive velocities for target stars within 190 pc of the sun, and bothpositive and negative velocities for more distant target stars,confirming an earlier prediction by Cowie, Songaila, and York (1979).The nearby positive velocity cloud, designated here as Orion-Lepus 70(OL 70), is a standard diffuse interstellar cloud: it is subject to theambient galactic radiation field, with properties consistent with Tabout equal to 100 K and n about equal to 3/cu cm. Combined with acolumn density log N(H) = 19.8-20.0/sq cm, these values imply a cloudthickness of about 7 pc. The kinematics of OL 70 are consistent witheither an origin as part of the expanding Loop I superbubble shell, oras part of Lindbald's expanding ring, or a synthesis of the two models.The negative velocity interstellar components seen in stars at d notless than 200 pc are caused by interstellar matter accelerated by theexpanding Ori-Eri superbubble. Relatively dense interstellar gas atpositive LSR velocities is also found within the Orion association, sothat it is difficult to pick out OL 70 components in the spectra of thedistant stars.
| 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.
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| Сазвежђа: | Орион |
| Ректацензија: | 05h35m26.75s |
| Deклинација: | -08°38'44.1" |
| Apparent магнитуда: | 8.129 |
| Даљина: | 334.448 parsecs |
| Proper motion RA: | -21.5 |
| Proper motion Dec: | -0.6 |
| B-T magnitude: | 8.12 |
| V-T magnitude: | 8.129 |
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