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POX 52: A Dwarf Seyfert 1 Galaxy with an Intermediate-Mass Black Hole
We describe new optical images and spectra of POX 52, a dwarf galaxywith an active nucleus that was originally detected in the POXobjective-prism survey. While POX 52 was originally thought to be aSeyfert 2 galaxy, the new data reveal an emission-line spectrum verysimilar to that of the dwarf Seyfert 1 galaxy NGC 4395, with broadcomponents to the permitted line profiles, and we classify POX 52 as aSeyfert 1 galaxy. The host galaxy appears to be a dwarf elliptical, andits brightness profile is best fit by a Sérsic model with anindex of 3.6+/-0.2 and a total magnitude of MV=-17.6.Applying mass-luminosity-line width scaling relations to estimate theblack hole mass from the broad Hβ line width and nonstellarcontinuum luminosity, we findMBH~1.6×105Msolar. The stellarvelocity dispersion in the host galaxy, measured from the Ca IIλ8498, 8542 lines, is 36+/-5 km s-1, also suggestiveof a black hole mass of order 105Msolar. Furthersearches for active nuclei in dwarf galaxies can provide uniqueconstraints on the demographics of black holes in the mass range below106Msolar.
| Mesures de vitesses radiales. VIII. Accompagnement AU sol DU programme d'observation DU satellite HIPPARCOS
We publish 1879 radial velocities of stars distributed in 105 fields of4^{\circ} \times 4^{\circ}. We continue the PPO series \cite[(Fehrenbachet al. 1987;]{Feh87} \cite[Duflot et al. 1990, 1992 and 1995),]{Du90}using the Fehrenbach objective prism method. Table 1 only available inelectronic form at CDS via to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/Abstract.html
| Vitesses radiales. Catalogue WEB: Wilson Evans Batten. Subtittle: Radial velocities: The Wilson-Evans-Batten catalogue.
We give a common version of the two catalogues of Mean Radial Velocitiesby Wilson (1963) and Evans (1978) to which we have added the catalogueof spectroscopic binary systems (Batten et al. 1989). For each star,when possible, we give: 1) an acronym to enter SIMBAD (Set ofIdentifications Measurements and Bibliography for Astronomical Data) ofthe CDS (Centre de Donnees Astronomiques de Strasbourg). 2) the numberHIC of the HIPPARCOS catalogue (Turon 1992). 3) the CCDM number(Catalogue des Composantes des etoiles Doubles et Multiples) byDommanget & Nys (1994). For the cluster stars, a precise study hasbeen done, on the identificator numbers. Numerous remarks point out theproblems we have had to deal with.
| MK classification and photometry of stars used for time and latitude observations at Mizusawa and Washington
MK spectral classifications are given for 591 stars which are used fortime and latitude observations at Mizusawa and Washington. Theclassifications in the MK system were made by slit spectrograms ofdispersion 73 A/mm at H-gamma which were taken with the 91 cm reflectorat the Okayama Astrophysical Observatory. Photometric observations in UBV were made with the 1-meter reflector at the Flagstaff Station of U.S.Naval Observatory. The spectrum of HD 139216 was found to show a strongabsorption line of H-beta. The following new Am stars were found:HD9550, 25271, 32784, 57245, 71494, and 219109. The following new Apstars were found: HD6116, 143806, 166894, 185171, and 209260. The threestars, HD80492, 116204, and 211376, were found to show the emission inCaII H and K lines.
| Star catalogs for the Washington and Richmond photographic zenith tubes.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1973AJ.....78..642M&db_key=AST
| UBV Photometry of 173 PZT Stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1971PASP...83..177W&db_key=AST
| Radial Velocities, Spectral Types, and Luminosity Classes of 820 Stars.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1950ApJ...112...48M&db_key=AST
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| Takýmyýldýz: | Kertenkele |
| Sað Açýklýk: | 22h17m49.94s |
| Yükselim: | +39°01'33.6" |
| Görünürdeki Parlaklýk: | 7.4 |
| Uzaklýk: | 212.766 parsek |
| özdevim Sað Açýklýk: | 68.6 |
| özdevim Yükselim: | 15.7 |
| B-T magnitude: | 8.985 |
| V-T magnitude: | 7.531 |
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