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...-024, [[Gliese-Jahreiss catalogue|Gliese]] 699, [[Hipparcos Catalogue|HIP]] 87937, [[Luyten Five-Tenths catalogue|LFT]] 1385, [[Luyten Half ...ius]] (the brightest star in the night sky) and 6 for the faintest visible objects (the scale is [[logarithmic scale|logarithmic]], and so magnitude 9.57 is o ...

...;3278.00, [[Gliese-Jahreiss catalogue|GJ]]&nbsp;551, [[Hipparcos catalogue|HIP]]&nbsp;70890, [[Luyten Five-Tenths catalogue|LFT]]&nbsp;1110, [[Luyten Half ...ed detection by the radial velocity method.</ref> The detection of smaller objects will require the use of new instruments, such as the proposed [[Space Inter ...

...n Space Agency, 1997, and the [http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HIP%2032349 entry for Sirius] in the Hipparcos catalogue ([[Centre de Données a ...Half-Second catalogue|LHS]] 219, ADS 5423, LTT 2638, [[Hipparcos catalogue|HIP]] 32349. <br />'''B''': EGGR 49, WD 0642-166.<ref name=simbada /><ref name= ...

...servatory Star Catalog|SAO 147986]], LPM 84, FK5 59, [[Hipparcos catalogue|HIP 8102]].<ref name="SIMBAD"/> }} ..., determined by comparing its position relative to more distant background objects. Tau Ceti is considered to be a high-proper-motion star, although it only h ...

...hsonian Astrophysical Observatory|SAO&nbsp;107138]], [[Hipparcos catalogue|HIP&nbsp;105860]].<ref name="simbad" /> | booktitle =The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings ...

...Astrophysical Observatory Star Catalog|SAO 67174]], [[Hipparcos catalogue|HIP 91262]].<ref name=SIMBAD/> }} ...stellar disk of dust. This dust is likely the result of collisions between objects in an orbiting [[debris disk]], which is analogous to the [[Kuiper belt]] i ...