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Spectroscopic analysis of southern B and Be stars
Spectroscopic monitoring of 141 southern field B-type stars, 114 of themknown to exhibit the Be phenomenon, allowed the estimation of theirprojected rotational velocities, effective temperatures and superficialgravities from both line and equivalent width fitting procedures.Stellar ages, masses and bolometric luminosities were derived frominternal structure models. Without taking into account the effects ofgravity darkening, we note the occurrence of the Be phenomenon in laterstages of main-sequence phase.
| Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics
The Catalogue, available at the Centre de Données Stellaires deStrasbourg, consists of 13 573 records concerning the results obtainedfrom different methods for 7778 stars, reported in the literature. Thefollowing data are listed for each star: identifications, apparentmagnitude, spectral type, apparent diameter in arcsec, absolute radiusin solar units, method of determination, reference, remarks. Commentsand statistics obtained from CADARS are given. The Catalogue isavailable in electronic form at the CDS via anonymous ftp tocdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcar?J/A+A/367/521
| The Edinburgh-Cape Blue Object Survey - I. Description of the survey
The Edinburgh-Cape Blue Object Survey is a major survey to discover bluestellar objects brighter than B~18 in the southern sky. It is planned tocover an area of sky of 10000 deg^2 with --b-->30 deg and delta<0deg. The blue stellar objects are selected by automatic techniques fromU and B pairs of UK Schmidt Telescope plates scanned with the COSMOSmeasuring machine. Follow-up photometry and spectroscopy are beingobtained with the SAAO telescopes to classify objects brighter thanB=16.5. This paper describes the survey, the techniques used to extractthe blue stellar objects, the photometric methods and accuracy, thespectroscopic classification, and the limits and completeness of thesurvey.
| Magnetic fields around BOK globules: CCD polarimetry of CB 4
The small Bok globule CB 4 was probed using a CCD imaging polarimeter inorder to create a detailed map of the magnetic field associated withthis cloud. Stars as faint as 17th mag at V band were measuredpolarimetrically with uncertainties less than 1%. Sky transmissionvariations were minimized via a system of synchronous polaroid rotationand bidirectional charge shifting. In all, 80 stars behind the peripheryof the globule were accurately analyzed polarimetrically. Thelarge-scale (1-2 pc) magnetic field direction around CB 4 was found tobe very uniform (P.A. = 63.3 deg +/- 1.1 deg). Double-Gaussian fittingof the polarization position angle histogram gave a dispersion of 10 degabout the primary field direction. Possible field-line compression wasfound inward of approximately 0.2 pc from the cloud center. Noappreciable twisting of field lines was found. By plotting stellarseparations against differences of polarization angles, CB 4 was foundto have a magnetic field decorrelation length of approximately 0.1 pc,similar to the size of the visually opaque cire, but much smaller thanthe size of the bright optical rim or CO half-power contour ofapproximately 0.5 pc. The magnetic field decorrelation length may berelated to a characteristic transient clumping size, or perhaps even toclumps of a more permanent nature.
| Broad-band photometry of selected southern ultraviolet-bright stars.
Not Available
| Effective temperatures, radii, and luminosities of O emission, Be and AE stars
Dereddened fluxes, together with the ultraviolet measurements ofThompson et al. (1978), have been compared with those of Kurucz's (1979)model atmospheres to derive effective temperatures of some O-emission,Be and Ae stars. With the measured monochromatic fluxes, their angulardiameters and luminosities were determined. It is found that themajority of the stars are cooler than the Zero-Age Main Sequence (ZAMS),suggesting that they are slightly more evolved than ZAMS stars.
| 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.
| A Catalogue of Be-Stars
Not Available
| Observations of southern emission-line stars
A catalog of 1929 stars showing H-alpha emission on photographic platesis presented which covers the entire southern sky south of declination-25 deg to a red limiting magnitude of about 11.0. The catalog providesprevious designations of known emission-line stars equatorial (1900) andgalactic coordinates, visual and photographic magnitudes, H-alphaemission parameters, spectral types, and notes on unusual spectralfeatures. The objects listed include 16 M stars, 25 S stars, 37 carbonstars, 20 symbiotic stars, 40 confirmed or suspected T Tauri stars, 16novae, 14 planetary nebulae, 11 P Cygni stars, 9 Bep stars, 87 confirmedor suspected Wolf-Rayet stars, and 26 'peculiar' stars. Two new Tassociations are discovered, one in Lupus and one in Chamaeleon. Objectswith variations in continuum or H-alpha intensity are noted, and thedistribution by spectral type is analyzed. It is found that the skydistribution of these emission-line stars shows significantconcentrations in the region of the small Sagittarius cloud and in theCarina region.
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| Takýmyýldýz: | Irmak |
| Sað Açýklýk: | 04h38m16.17s |
| Yükselim: | -24°39'30.8" |
| Görünürdeki Parlaklýk: | 8.549 |
| Uzaklýk: | 1020.408 parsek |
| özdevim Sað Açýklýk: | 2.3 |
| özdevim Yükselim: | 5 |
| B-T magnitude: | 8.417 |
| V-T magnitude: | 8.539 |
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