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The Carina Spiral Feature: Strömgren-Hβ photometry approach. I. The photometric data-base
A data-base collating all uvbybeta photometry available at present forO-B9 stars brighter than 10th visual magnitude in the field of theCarina Spiral Feature is presented. The completeness and homogeneity ofthe data-base are discussed.Based on CDS data.Table 1 is only available in electronic form at the CDS via anonymousftp to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/410/523
| The calibration of the Stromgren photometric system for A, F and early G supergiants. I - The observational data
An empirical calibration of the Stromgren uvby-beta photometric systemfor the A, F, and early G supergiants is being derived. This paperexplains the observational program and the photometric reductiontechniques used and presents a catalog of new Stromgren photometry forover 600 A, F, and G supergiants.
| The WN4 + O4-6 Wolf-Rayet binary HD 90657
HD 90657 is shown to be a WN4 + O4-6 binary, much like the WN4 + O9binary HD 186943 with mass ratio M(W-R)/M(O) approximately equal to0.52. The best W-R orbit is derived from the emission lines of highestexcitation, which show the least phase shift relative to the (reliable)absorption-line orbit due to the O component. Light curve variationsrestrain the masses to a range of about 11-14 solar masses for the WN4component, and 21-28 solar masses for the O-type component
| 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.
| A catalogue of new H-alpha emission stars in the eta Carinae nebula region.
Not Available
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Besorolás csoportokba:
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Pozíciós és asztrometriai adatok
| Csillagkép: | Hajógerinc |
| Rektaszcenzió: | 10h25m16.19s |
| Deklináció: | -58°52'20.9" |
| Vizuális fényesség: | 6.996 |
| Távolság: | 259.067 parszek |
| RA sajátmozgás: | -17.1 |
| Dec sajátmozgás: | 6.6 |
| B-T magnitude: | 6.879 |
| V-T magnitude: | 6.987 |
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