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Re: [vsnet-chat 6488] 93 comp star for RS Oph > I wish I could use it! > Anyway, let me clarify that my concern regarding variability of HD 162215 > wasn't based on Arne's previous deeper data (I supposed it could be a > saturated measure) but in a V measure in the GCPD: > V= 9.68, B-V= 1.266. > This is from Connelley M., and Sandage A., Photoelectric observations of RS > Ophiuchi, 1978, PASP 70, 600. > Arne's measure gained another meaning after I saw that measure.... > But.... > ASAS-3 data don't support variability. And now Arne has obtained a > consistent result with Tycho-2 and ASAS-3, so... I think it could be used as > a comparison star as Mike suggested. > > Of course, now the charts are issued, an eclipse or something will happen ;-)) > BTW it is a single-lined spectroscopic binary (Latham, 2002). Is this K0 star a dwarf or a giant? I noticed that there is a possible Einstein EMSS2 detection located close to this star. 175014.4 -064812 (2000.0) 2.32sigma By taking the typical uncertainties of Einstein detections in this field, this detection may correspond to this star itself. Could someone enlighten us more? Regards, Taichi Kato
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
