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Statistical Constraints for Astrometric Binaries with Nonlinear Motion
Useful constraints on the orbits and mass ratios of astrometric binariesin the Hipparcos catalog are derived from the measured proper motiondifferences of Hipparcos and Tycho-2 (Δμ), accelerations ofproper motions (μ˙), and second derivatives of proper motions(μ̈). It is shown how, in some cases, statistical bounds can beestimated for the masses of the secondary components. Two catalogs ofastrometric binaries are generated, one of binaries with significantproper motion differences and the other of binaries with significantaccelerations of their proper motions. Mathematical relations betweenthe astrometric observables Δμ, μ˙, and μ̈ andthe orbital elements are derived in the appendices. We find a remarkabledifference between the distribution of spectral types of stars withlarge accelerations but small proper motion differences and that ofstars with large proper motion differences but insignificantaccelerations. The spectral type distribution for the former sample ofbinaries is the same as the general distribution of all stars in theHipparcos catalog, whereas the latter sample is clearly dominated bysolar-type stars, with an obvious dearth of blue stars. We point outthat the latter set includes mostly binaries with long periods (longerthan about 6 yr).
| Speckle Interferometry of New and Problem Hipparcos Binaries. II. Observations Obtained in 1998-1999 from McDonald Observatory
The Hipparcos satellite made measurements of over 9734 known doublestars, 3406 new double stars, and 11,687 unresolved but possible doublestars. The high angular resolution afforded by speckle interferometrymakes it an efficient means to confirm these systems from the ground,which were first discovered from space. Because of its coverage of adifferent region of angular separation-magnitude difference(ρ-Δm) space, speckle interferometry also holds promise toascertain the duplicity of the unresolved Hipparcos ``problem'' stars.Presented are observations of 116 new Hipparcos double stars and 469Hipparcos ``problem stars,'' as well as 238 measures of other doublestars and 246 other high-quality nondetections. Included in these areobservations of double stars listed in the Tycho-2 Catalogue andpossible grid stars for the Space Interferometry Mission.
| Lithium in high velocity A and F stars: Constraints on the blue straggler phenomenon
We have determined equivalent widths for a number of atomic lines,including the lambda 6707 resonance doublet of Li, from spectra of asample of candidate early-type high-velocity stars (including a numberof blue straggler candidates) and low-velocity comparison stars. We findthat the high-velocity candidates can be divided into three distinctgroups: (1) stars with low abundances both of Li and of metals ingeneral; (2) stars with low abundances of Li but only slightdeficiencies of the other metals; and (3) stars with nearly normalamounts of both Li and other metals. We tentatively identify thesegroups as (1) halo and thick-disk blue stragglers; (2) old, thinnishdisk blue stragglers; and (3) nearly normal Population l stars whichprobably lie in the tail of the usual Pop. l velocity distribution. Thekinematic properties of the three groups are consistent with thisinterpretation. Li is a fragile element which is easily destroyed in thehot interiors of main-sequence stars, and has previously been shown tobe depleted in the atmospheres of blue stragglers in the open clusterM67. Our results on objects that we have identified in this paper asold, halo or thick disk, field blue stragglers suggest that lithiumdepletion is a general property of blue stragglers; this argues thatlarge scale mixing must be a part of any mechanism that produces bluestragglers. Our observations of low lithium abundances in a number ofmetal-normal, high-velocity, A stars, suggest that the high-latitude Astars observed by Rodgers an d collaborators are probably not producedin the collison of a Magellanic Cloud-like object with the Galactic diskin the past few Gyr. A more likely hypothesis (that is consistent withour lithium abundances) is that the high latitude, normal gravity,metal-rich, A star population consists primarily of blue stragglers.These data also have allowed a redetermination of the relationshipbetween the Stromgren metallicity index delta mo and (M/H)for low-metallicity objects.
| Early type high-velocity stars in the solar neighborhood. IV - Four-color and H-beta photometry
Results are presented from photometric obaservations in the Stromgrenuvby four-color and H-beta systems of early-type high-velocity stars inthe solar neighborhood. Several types of photometrically peculiar starsare selected on the basis of their Stromgren indices and areprovisionally identified as peculiar A stars, field horizontal-branchstars, metal-poor stars near the Population II and old-disk turnoffs,metal-poor blue stragglers, or metallic-line A stars. Numerousphotometrically normal stars were also found.
| Early-type high-velocity stars in the solar neighborhood. I - List of candidates
Suspected nearby high-velocity stars of spectral types B and A areidentified by their proper motions, which are generally too small forthe stars to have been included in previous catalogs of high-velocitystars. The same selection process is then extended to spectral type Fstars, in order to both provide a companion sample and investigatewhether the hypothetical high-velocity, metal-rich population continuesto later spectral types. Of the presented list of 371 stars withconfirmed proper motions, 168 are of A and B spectral types. Photometricand spectroscopic observations of these stars are required to eliminatethose with misclassified spectra and convert proper motions into spacevelocities. The identification of type of stars is important forunderstanding apparent exceptions to the correlation between stellarages, metal abundances, and kinematic properties.
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| Takýmyýldýz: | Kanatli At |
| Sað Açýklýk: | 23h56m04.90s |
| Yükselim: | +14°50'32.5" |
| Görünürdeki Parlaklýk: | 8.295 |
| Uzaklýk: | 136.612 parsek |
| özdevim Sað Açýklýk: | 66.7 |
| özdevim Yükselim: | 34.8 |
| B-T magnitude: | 8.616 |
| V-T magnitude: | 8.322 |
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