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Fundamental parameters of Be stars located in the seismology fields of COROT
In preparation for the COROT space mission, we determined thefundamental parameters (spectral type, temperature, gravity, V sin i) ofthe Be stars observable by COROT in its seismology fields (64 Be stars).We applied a careful and detailed modeling of the stellar spectra,taking into account the veiling caused by the envelope, as well as thegravitational darkening and stellar flattening due to rapid rotation.Evolutionary tracks for fast rotators were used to derive stellar massesand ages. The derived parameters will be used to select Be stars assecondary targets (i.e. observed for 5 consecutive months) and short-runtargets of the COROT mission. Furthermore, we note that the main part ofour stellar sample falls in the second half of the main sequence lifetime, and that in most cases the luminosity class of Be stars isinaccurate in characterizing their evolutionary status.
| Physical Parameters of Southern B- and Be-Type Stars
In this paper we present new results on stellar fundamental parametersfor early B and Be field stars observed in the southern hemisphere:effective temperature, superficial gravity, and projected stellarrotation velocity. The estimation of their projected rotation velocitiesis made by two successive methods. We first obtain an initial valuebased on Fourier transforms of the He I λ4471 line for 34 B andBe field stars with magnitudes in the range0.5<=mv<=10, followed by a more accurate fittingprocedure of observed lines with non-LTE model line profiles. Thisprocedure yields stellar rotation velocity estimates that are inagreement with those of the literature. We derive also Teffand logg values by fitting equivalent widths and profiles of NLTE modelspectra to the observed ones. Finally, we give estimates of stellarages, masses, and bolometric luminosities derived from interpolations inthe evolutionary tracks calculated by Schaller.
| Catalogue of H-alpha emission stars in the Northern Milky Way
The ``Catalogue of Stars in the Northern Milky Way Having H-alpha inEmission" appears in Abhandlungen aus der Hamburger Sternwarte, Band XIin the year 1997. It contains 4174 stars, range {32degr <= l() II< 214degr , -10degr < b() II < +10degr } having the Hαline in emission. HBH stars and stars of further 99 lists taken from theliterature till the end of 1994 were included in the catalogue. We givethe cross-identification of stars from all lists used. The catalogue isalso available in the Centre de Données, Strasbourg ftp130.79.128.5 or http://cdsweb.u-strasbg.fr and at the HamburgObservatory via internet.
| Open clusters with Hipparcos. I. Mean astrometric parameters
New memberships, mean parallaxes and proper motions of all 9 openclusters closer than 300 pc (except the Hyades) and 9rich clusters between 300 and 500 pc have been computed using Hipparcosdata. Precisions, ranging from 0.2 to 0.5 mas for parallaxes and 0.1 to0.5 mas/yr for proper motions, are of great interest for calibratingphotometric parallaxes as well as for kinematical studies. Carefulinvestigations of possible biases have been performed and no evidence ofsignificant systematic errors on the mean cluster parallaxes has beenfound. The distances and proper motions of 32 more distant clusters,which may be used statistically, are also indicated. Based onobservations made with the ESA Hipparcos astrometry satellite
| Catalogue of stars in the northern Milky Way having H-alpha in emission
Not Available
| Distances, reddenings and distribution of emission B-stars in the galactic centre region /l/ not greater than 45 deg
The distribution of Be stars in the region surrounding the Galacticcenter and their correlation to the spiral structure of the Galaxy hasbeen studied. The results are discussed in terms of reddenings anddistances of these stars. Data are presented on the Galacticcoordinates, colors, interstellar color excesses, reddening-freemagnitudes and colors, adopted absolute magnitudes, distances in kpc,distances from the Galactic plane, and MK spectral type.
| Photometric observations of emission B-stars in the southern Milky Way
In order to study the distribution of Be stars and their correlation tothe local spiral structure of the Galaxy photoelectric UBV photometrywas carried out for a total of 488 Be stars located in the southernMilky Way between galactic longitudes 315 and 45 deg. UBV magnitudes arepresented for these stars.
| Photoelectric photometry of early-type stars in a field in Ophiuchus
Not Available
| Axial Rotation in the Later B-Type Emission-Line Stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1966ApJ...145..121S&db_key=AST
| A Peculiar Emission Star in Cygnus, MHα 328-116
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1966ApJ...144.1135F&db_key=AST
| Second Supplement to the Mount Wilson Catalogue and Bibliography of Stars of Classes B and a whose Spectra have Bright Hydrogen Lines.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1949ApJ...110..387M&db_key=AST
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Datos observacionales y astrométricos
| Constelación: | Serpente |
| Ascensión Recta: | 18h33m17.84s |
| Declinación: | +05°26'43.9" |
| Magnitud Aparente: | 7.651 |
| Distancia: | 444.444 parsecs |
| Movimiento Propio en Ascensión Recta: | -1.9 |
| Movimiento Propio en Declinación: | -7.1 |
| B-T magnitude: | 7.846 |
| V-T magnitude: | 7.668 |
Catálogos y designaciones:
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