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A Method for Determining the Physical Properties of the Coldest Known Brown Dwarfs
We present a method for measuring the physical parameters of the coldestT-type brown dwarfs using low-resolution near-infrared spectra. Bycomparing H2O and H2-sensitive spectral ratiosbetween empirical data and theoretical atmosphere models, andcalibrating these ratios to measurements for the well-characterized 2-5Gyr companion brown dwarf Gliese 570D, we derive estimates of theeffective temperatures and surface gravities for 13 mid- and late-typefield T dwarfs. We also deduce the first quantitative estimate ofsubsolar metallicity for the peculiar T dwarf 2MASS 0937+2931. Derivedtemperatures are consistent with prior estimates based on parallax andbolometric luminosity measurements, and examination of possiblesystematic effects indicate that the results are robust. Two recentlydiscovered late-type T dwarfs, 2MASS 0939-2448 and 2MASS 1114-2618, bothappear to be >~50 K cooler than the latest type T dwarf, 2MASS0415-0935, and are potentially the coldest and least luminous browndwarfs currently known. We find that, in general, higher surface gravityT dwarfs have lower effective temperatures and luminosities for a givenspectral type, explaining previously observed scatter in theTeff/spectral type relation for these objects. Masses, radii,and ages are estimated for the T dwarfs in our sample using theevolutionary models of Burrows et al.; we also determine masses andradii independently for eight T dwarfs with measured luminosities. Thesetwo determinations are largely consistent, lending support to thevalidity of evolutionary models at late ages. Our method is well suitedto large samples of faint brown dwarfs and can ultimately be used todirectly measure the substellar mass function and formation history inthe Galaxy.
| Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS
Radial velocities have been determined for a sample of 2930 B2-F5 stars,95% observed by the Hipparcos satellite in the north hemisphere and 80%without reliable radial velocity up to now. Observations were obtainedat the Observatoire de Haute Provence with a dispersion of 80Ä,mm(-1) with the aim of studying stellar and galactic dynamics.Radial velocities have been measured by correlation with templates ofthe same spectral class. The mean obtained precision is 3.0 km s(-1)with three observations. A new MK spectral classification is estimatedfor all stars. Based on observations made at the Haute ProvenceObservatory, France and on data from The Hipparcos Catalogue, ESA.Tables 4, 5 and 6 are only available in electronic form at the CDS viaanonymous ftp to cdsarc.u-strasbg.fr or viahttp://cdsweb.u-strasbg.fr/Abstract.htm
| UvbyHbeta_ photometry of main sequence A type stars.
We present Stroemgren uvby and Hbeta_ photometry for a set of575 northern main sequence A type stars, most of them belonging to theHipparcos Input Catalogue, with V from 5mag to 10mag and with knownradial velocities. These observations enlarge the catalogue we began tocompile some years ago to more than 1500 stars. Our catalogue includeskinematic and astrophysical data for each star. Our future goal is toperform an accurate analysis of the kinematical behaviour of these starsin the solar neighbourhood.
| Vacuum ultraviolet imagery of the Virgo cluster region
The results are reported of an experiment using the UV imager aboard anattitude-controlled S520 type sounding rocket. The total UV fluxes ofgalaxies in the Virgo Cluster as well as the flux level of the diffuseUV background around the cluster were measured. The data on NGC 4486 andNGC 4472 confirm the variation in the degree of the 'turnup' below 200nm in the energy spectrum of the total light of elliptical galaxies. Attwo-color diagram of galaxies of visual/near-UV/vacuum UV indicates thatcolors of spiral galaxies are distributed within a strip andwell-correlated with the morphological type, while elliptical galaxiesare located differently from spiral galaxies.
| The galactic reddening law - The evidence from uvby-beta photometry of B stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1985A&A...142..189T&db_key=AST
| Four-colour photometry of B stars north of B = + 45 deg and comparison with the south
Four-color photometry of 33 Henry Draper B stars north of b = + 45 degis presented. Most are little-reddened B or intermediate-A stars. A newAm star is discovered. The new measures essentially complete uvbyphotometry of all HD B stars within 45 deg of either galactic pole. Thenorthern and southern cones of HD B stars are compared, and selectioneffects deduced. Far from the galactic plane, it appears that B starsmay be equally distributed north and south of the plane; closer to thesun, an asymmetry associated with Gould's Belt is evident.
| Photoelectric UBV observations made on the Palomar 20-inch telescope
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1973MNRAS.164..133P&db_key=AST
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Besorolás csoportokba:
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Pozíciós és asztrometriai adatok
| Csillagkép: | Szűz |
| Rektaszcenzió: | 13h26m58.94s |
| Deklináció: | +11°54'30.8" |
| Vizuális fényesség: | 7.992 |
| Távolság: | 251.256 parszek |
| RA sajátmozgás: | 2.2 |
| Dec sajátmozgás: | -4.1 |
| B-T magnitude: | 7.979 |
| V-T magnitude: | 7.991 |
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