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HD 99317


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מאמרים קשורים

The High Angular Resolution Multiplicity of Massive Stars
We present the results of a speckle interferometric survey of Galacticmassive stars that complements and expands upon a similar survey madeover a decade ago. The speckle observations were made with the Kitt PeakNational Observatory and Cerro Tololo Inter-American Observatory 4 mtelescopes and USNO speckle camera, and they are sensitive to thedetection of binaries in the angular separation regime between 0farcs03and 5'' with relatively bright companions (ΔV < 3). We reporton the discovery of companions to 14 OB stars. In total we resolvedcompanions of 41 of 385 O-stars (11%), 4 of 37 Wolf-Rayet stars (11%),and 89 of 139 B-stars (64%; an enriched visual binary sample that weselected for future orbital determinations). We made a statisticalanalysis of the binary frequency among the subsample that are listed inthe Galactic O Star Catalog by compiling published data on other visualcompanions detected through adaptive optics studies and/or noted in theWashington Double Star Catalog and by collecting published informationon radial velocities and spectroscopic binaries. We find that the binaryfrequency is much higher among O-stars in clusters and associationscompared to the numbers for field and runaway O-stars, consistent withpredictions for the ejection processes for runaway stars. We present afirst orbit for the O-star δ Orionis; a linear solution of theclose, apparently optical, companion of the O-star ι Orionis; andan improved orbit of the Be star δ Scorpii. Finally, we listastrometric data for another 249 resolved and 221 unresolved targetsthat are lower mass stars that we observed for various other scienceprograms.

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תצפית ומידע אסטרומטרי

קבוצת-כוכבים:זבוב
התרוממות ימנית:11h24m48.90s
סירוב:-67°07'47.5"
גודל גלוי:7.762
מרחק:298.507 פארסק
תנועה נכונה:-14.2
תנועה נכונה:0.4
B-T magnitude:7.885
V-T magnitude:7.773

קטלוגים וכינוים:
שם עצם פרטי   (Edit)
HD 1989HD 99317
TYCHO-2 2000TYC 8971-277-1
USNO-A2.0USNO-A2 0225-11245900
HIPHIP 55702

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