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Herbig Ae/Be Stars in nearby OB Associations
We have carried out a study of the early-type stars in nearby OBassociations spanning an age range of ~3-16 Myr, with the aim ofdetermining the fraction of stars that belong to the Herbig Ae/Be class.We studied the B, A, and F stars in the nearby (<=500 pc) OBassociations Upper Scorpius, Perseus OB2, Lacerta OB1, and Orion OB1,with membership determined from Hipparcos data. We also included in ourstudy the early-type stars in the Trumpler 37 cluster, part of the CepOB2 association. We obtained spectra for 440 Hipparcos stars in theseassociations, from which we determined accurate spectral types, visualextinctions, effective temperatures, luminosities and masses, usingHipparcos photometry. Using colors corrected for reddening, we find thatthe Herbig Ae/Be stars and the classical Be (CBe) stars occupy clearlydifferent regions in the JHK diagram. Thus, we use the location on theJHK diagram, as well as the presence of emission lines and of strong 12μm flux relative to the visual, to identify the Herbig Ae/Be stars inthe associations. We find that the Herbig Ae/Be stars constitute a smallfraction of the early-type stellar population even in the youngerassociations. Comparing the data from associations with different agesand assuming that the near-infrared excess in the Herbig Ae/Be starsarises from optically thick dusty inner disks, we determined theevolution of the inner disk frequency with age. We find that the innerdisk frequency in the age range 3-10 Myr in intermediate-mass stars islower than that in the low-mass stars (<1 Msolar) inparticular, it is a factor of ~10 lower at ~3 Myr. This indicates thatthe timescales for disk evolution are much shorter in theintermediate-mass stars, which could be a consequence of more efficientmechanisms of inner disk dispersal (viscous evolution, dust growth, andsettling toward the midplane).
| IRAS 05436-0007 and the Emergence of MCNeil's Nebula
We present a study of McNeil's Nebula, a newly appeared reflectionnebula in the L1630 cloud, together with photometry and spectroscopy ofits source. New IR photometry compared with earlier Two Micron All SkySurvey data shows that the star has brightened by about 3 mag in thenear-infrared, changing its location in a J-H/H-K' diagramprecisely along a reddening vector. A Gemini Near InfraRed Imager K-bandspectrum shows strong CO band head emission, and Brγ is inemission, indicative of strong accretion. A Gemini Multi-ObjectSpectrograph optical spectrum shows only a red, heavily veiledcontinuum, with Hα strongly in emission and displaying apronounced P Cygni profile, with an absorption trough reachingvelocities up to 600 km s-1. This implies significant massloss in a powerful wind. However, no evidence is found for any shocks,as commonly seen in collimated outflows from young stars. Apparently theeruption has dispersed a layer of extinction, and this, together withthe intrinsic brightening of the IRAS source, has allowed an earlieroutflow cavity to be flooded with light, thus creating McNeil's Nebula.
| 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
| Far-ultraviolet stellar photometry: A field in Orion
Far-ultraviolet photometry for 625 objects in Orion is presented. Thesedata were extracted from electrographic camera images obtained duringsounding rocket flights in 1975 and 1982. The 1975 images were centeredclose to the belt of Orion while the 1982 images were centeredapproximately 9 deg further north. One hundred and fifty stars fell inthe overlapping region and were observed with both cameras. Sixty-eightpercent of the objects were tentatively identified with known starsusing the SIMBAD database while another 24% are blends of objects tooclose together to separate with our resolution. As in previous studies,the majority of the identified ultraviolet sources are early-type stars.However, there are a significant number for which no such identificationwas possible, and we suggest that these are interesting objects whichshould be further investigated. Seven stars were found which were brightin the ultraviolet but faint in the visible. We suggest that some ofthese are nearby white dwarfs.
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| Takýmyýldýz: | Avci |
| Sað Açýklýk: | 05h55m57.32s |
| Yükselim: | +00°50'10.1" |
| Görünürdeki Parlaklýk: | 7.168 |
| Uzaklýk: | 172.117 parsek |
| özdevim Sað Açýklýk: | -1.6 |
| özdevim Yükselim: | 1 |
| B-T magnitude: | 7.309 |
| V-T magnitude: | 7.18 |
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