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HD 92127


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Ýlgili Makaleler

Period Change and Surface Activity of the Eclipsing Binary UV Leonis
From Johnson B and V photometric measurements of V=8.98 mag eclipsingbinary UV Leonis we calculated the epochs of primary and secondaryminima, which we used to complement the published O-C catalog by Kreineret al. (2000). From this we give a brief analysis of the observed periodchange and give qualitative presumptions about the physics that mighthave caused such a change. Further on, we use the observed systematicvertical shift in light curves as an indication of the surface activityof UV Leonis.

A Photometric Analysis and SPOT Model of the Detached Eclipsing Binary UV Leonis
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1996AJ....111.2081F&db_key=AST

Photoelectric Photometry of UZ Leonis
Not Available

Fluctuations dans les courbes de lumière de la variable à éclipses UV Leonis
Not Available

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Gözlemler ve gökölçümü verileri

Takýmyýldýz:Aslan
Sað Açýklýk:10h38m26.08s
Yükselim:+13°57'03.2"
Görünürdeki Parlaklýk:8.265
Uzaklýk:91.743 parsek
özdevim Sað Açýklýk:-5.5
özdevim Yükselim:-10.7
B-T magnitude:8.792
V-T magnitude:8.309

Kataloglar ve belirtme:
Özgün isimleri
HD 1989HD 92127
TYCHO-2 2000TYC 845-1154-1
USNO-A2.0USNO-A2 0975-06537847
HIPHIP 52070
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