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Chemically peculiar stars and their temperature calibration
Aims. The determination of effective temperature for chemically peculiar(CP) stars by means of photometry is a sophisticated task due to theirabnormal colours. Standard calibrations for normal stars lead toerroneous results and, in most cases corrections are necessary. Methods: In order to specify appropriate corrections, direct temperaturedeterminations for 176 objects of the different subgroups were collectedfrom the literature. This much larger sample than in previous studiestherefore allows a more accurate investigation, mostly based on averagetemperatures. Results: For the three main photometric systems (UBV,Geneva, Strömgren {uvby}β), methods to determine effectivetemperature are presented together with a comparison with formerresults. Based on the compiled data we provide evidence that He (CP4)objects also need a considerable correction, not noticed in formerinvestigations due to their small number. Additionally, a new relationfor the bolometric correction and the capability of standardcalibrations to deduce interstellar reddening for magnetic CP stars areshown.Tables 4 to 8 are only available in electronic form at http://www.aanda.org
| New Estimates of the Solar-Neighborhood Massive Star Birthrate and the Galactic Supernova Rate
The birthrate of stars of masses >=10 Msolar is estimatedfrom a sample of just over 400 O3-B2 dwarfs within 1.5 kpc of the Sunand the result extrapolated to estimate the Galactic supernova ratecontributed by such stars. The solar-neighborhood Galactic-plane massivestar birthrate is estimated at ~176 stars kpc-3Myr-1. On the basis of a model in which the Galactic stellardensity distribution comprises a ``disk+central hole'' like that of thedust infrared emission (as proposed by Drimmel and Spergel), theGalactic supernova rate is estimated at probably not less than ~1 normore than ~2 per century and the number of O3-B2 dwarfs within the solarcircle at ~200,000.
| Catalog of Galactic OB Stars
An all-sky catalog of Galactic OB stars has been created by extendingthe Case-Hamburg Galactic plane luminous-stars surveys to include 5500additional objects drawn from the literature. This work brings the totalnumber of known or reasonably suspected OB stars to over 16,000.Companion databases of UBVβ photometry and MK classifications forthese objects include nearly 30,000 and 20,000 entries, respectively.
| Properties of He-rich stars. II. CNO abundances and projected rotational velocities
We present an abundance analysis of light elements in the most massivechemically peculiar (CP) stars, He-rich stars. The analysis is based onboth low and high-resolution observations collected at ESO, La Silla,Chile in the optical region and includes 6 standard and 21 He-richstars. Light element abundances display a diverse pattern fromunder-solar up to above-solar values. Carbon is found underabundant inthe hottest He-rich stars and normal in the coolest ones, according tothe LTE model predictions. The distribution of projected rotationalvelocities shows a significant excess of slow rotators, no He-rich starshaving vsin i > 130 km s(-1) . Based on observations collected at theEuropean Southern Observatory, La Silla, Chile (programmes 7-043 and7-010 of periods 49 and 50 resp.)
| Light element abundances in He-rich stars
We present an abundance analysis of light elements in He-rich stars. Theanalysis is based on both low and high resolution observations collectedat ESO, La Silla, Chile in the optical region and includes 6 standardsand 21 He-rich stars. Light-element abundances display a diversepattern: they range from under-solar up to above-solar values.
| UBV beta Database for Case-Hamburg Northern and Southern Luminous Stars
A database of photoelectric UBV beta photometry for stars listed in theCase-Hamburg northern and southern Milky Way luminous stars surveys hasbeen compiled from the original research literature. Consisting of over16,000 observations of some 7300 stars from over 500 sources, thisdatabase constitutes the most complete compilation of such photometryavailable for intrinsically luminous stars around the Galactic plane.Over 5000 stars listed in the Case-Hamburg surveys still lackfundamental photometric data.
| Properties of He-rich stars. I. Their evolutionary state and helium abundance.
A determination of the surface gravity and an abundance analysis ofhelium in a sample of 17 He-rich and 5 normal, reference stars ispresented. These results are derived from low resolution CCD spectra,but each star was measured at least 6 times in order to obtain asignificant average spectrum for the spectroscopic variables. The heliumabundances derived from the models used are very close to 0.1 fornormal, reference stars and are larger for the others, clearlyindicating the He-rich phenomenon in them. NLTE effects, errors on themicroturbulence value or on the surface gravity do not influence theestimated helium abundances. Nevertheless, synthesized Geneva coloursare affected by the He-rich peculiarity, especially the [U-B] indexwhich systematically changes by -0.025 mag per 0.1 of He abundance forthe coolest stars in the sample. We cannot confirm the correlationbetween the evolutionary state and the helium abundance reportedpreviously (Zboril et al. 1994, International Conference on CP andMagnetic Stars.", Tatranska Lomnica, eds. J. Zverko and J. Ziznovsky, p.105), although we used a more reliable technique of log(g)determination. All He-rich objects lie within the main sequence: theirsurface gravities are all inside the range 4.1
| A spectroscopic database for Stephenson-Sanduleak Southern Luminous Stars
A database of published spectral classifications for objects in theStepenson-Sanduleak Luminous Stars in the Southern Milky Way catalog hasbeen compiled from the literature. A total of 6182 classifications for2562 stars from 139 sources are incorporated.
| Radio continuum emission from stars: a catalogue update.
An updated version of my catalogue of radio stars is presented. Somestatistics and availability are discussed.
| Radio emission from chemically peculiar stars
In five VLA observing runs the initial survey of radio emission frommagnetic Bp-Ap stars by Drake et al. is extended to include a total of16 sources detected at 6 cm out of 61 observed, giving a detection rateof 26 percent. Of these stars, three are also detected at 2 cm, four at3.6 cm, and five at 20 cm. The 11 new stars detected as radio sourceshave spectral types B5-A0 and are He-weak and Si-strong. No classical(SrCrEu-type) Ap stars have yet been detected. The 16 detected sourcesshow a wide range of radio luminosities with the early-B He-S stars onaverage 20 times more radio luminous than the late-B He-W stars and 1000times more luminous than Theta Aurigae. Multifrequency observationsindicate flat spectra in all cases. Four stars have a detectable degreeof circular polarization at one or more frequencies. It is argued thatthe radio-emitting CP (chemically peculiar) stars form a distinct classof radio stars that differs from both the hot star wind sources and theactive late-type stars. The observed properties of radio emission fromthese stars may be understood in terms of optically thickgyrosynchrotron emission from a nonthermal distribution of electronsproduced in a current sheet far from the star. In this model theelectrons travel along magnetic fields to smaller radii and highermagnetic latitudes where they mirror and radiate microwave radiation.
| 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.
| The discovery of nonthermal radio emission from magnetic Bp-Ap stars
In a VLA survey of chemically peculiar B- and A-type stars with strongmagnetic fields, five of the 34 stars observed have been identified as 6cm continuum sources. Three of the detections are helium-strong early Bpstars (Sigma Ori E, HR 1890, and Delta Ori C), and two are helium weak,silicon-strong stars with spectral types near A0p (IQ Aur = HD 34452,Babcock's star = HD 215441). The 6 cm luminosities L6 (ergs/s Hz) rangefrom log L6 = 16.2 to 17.9, somewhat less than the OB supergiants andW-R stars. Three-frequency observations indicate that the helium-strongBp stars are variable nonthermal sources.
| A survey of spectral morphology and rotational velocities among the helium-rich stars
A spectroscopically homogeneous listing of all known members of thehelium-rich B star category is presented together with uniform estimatesof their rotational velocities. Equivalent widths of hydrogen, helium,and metal lines in the spectra of the helium-rich and comparison starsare given. The distribution of rotational velocities is found to beindistinguishable from that of normal early B dwarfs, except for apossible excess of rapid rotators. The existence of metal abundanceanomalies in the helium-rich spectra is critically discussed, as is theidentification of helium-rich stars as massive Population I objects withnormal main sequence cores and surface helium enhancements, or as lowmass highly evolved objects with processed cores.
| UBV photometry for southern OB stars
New UBV photometry of 1227 OB stars in the southern Milky Way ispresented. For 1113 of these stars, MK spectral types have been reportedpreviously in a comprehensive survey to B = 10.0 mag.
| On the 4430 A interstellar band - A visual classification
A system of visual classification of the strength of the interstellarband 4430 A has been developed, based on spectra taken at spectralclassification dispersion. The intensity of the band was divided into 8main classes, defined by a group of selected standard stars. The systemwas applied to 1,111 southern OB stars contained in the catalog ofspectral types by Garrison, Hiltner, and Schild (1977). The mean errorin the classification was estimated to be plus or minus 1 class.Equivalent widths were measured for 100 stars; an excellent correlationwith the visual estimations was obtained. A calibration between thesetwo parameters is given.
| MK spectral classifications for southern OB stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1977ApJS...35..111G&db_key=AST
| UBV, Hbeta and polarization measurements of 1660 southern OB stars.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1977A&AS...27..215K&db_key=AST
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Pozíciós és asztrometriai adatok
| Csillagkép: | Nagy Kutya |
| Rektaszcenzió: | 07h12m02.29s |
| Deklináció: | -27°43'04.9" |
| Vizuális fényesség: | 9.246 |
| RA sajátmozgás: | -4.6 |
| Dec sajátmozgás: | 0.9 |
| B-T magnitude: | 9.026 |
| V-T magnitude: | 9.228 |
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