WDS 09354+3958 STF 1369 AB (DI Lyn) : NOTES
 
 
discov_num notes refcode
COU2084 A: DI Lyn. Aa is a 1.7d SB2.
Aa is also eclipsing binary DI Lyn (period 1.68154 day). Zas2010
A is SB1, P=438d Tok2014d
STF1369 AB: B component is 28d SB1. AB pair has an estimated period ~40,000y. Tok2006
SHY 542. Bayesian analysis by Shaya & Olling (2011) indicates very Shy2011
high (near 100%) probability pair is physical.
AB: H 4 30. MEv2010
 
 
REFERENCES
 
 
refcode metd author reference
MEv2010 - MacEvoy, B. ...................
MEv2010 private communication, 2010 (see http://www.handprint.com/ASTRO/index.html)
Shy2011 - Shaya, E.J. & Olling, R. 2011ApJS..192....2S
Shy2011 ApJS 192, 2, 2011
Shy2011 (Statistical analysis of probability that wide Hipparcos pairs are physical. Pairs
Shy2011 added to WDS only if probability 90% or greater.)
Tok2006 A j Tokovinin, A., Thomas, S., Sterzik, M., & Udry, S. 2006A&A...450..681T
Tok2006 +E2 A&A 450, 681, 2006
Tok2014d E2 - Tokovinin, A. 2014AJ....147...86T
Tok2014d AJ 147, 86, 2014
Zas2010 - Zasche, P. ...................
Zas2010 private communication, 2010
 
 
DISCOVERER
 
 
idgroup discov author
1 COU Couteau, P.
240 STF Struve, F.G.W.
 
 
WDS HISTORIC DATA
 
 
coord_2000 discov_num comp epoch obs pa sep mag_pri mag_sec spectr notes coord_arcsec_2000
09354+3958 STF1369 AB 2007 39 150 24.8 6.98 7.98 NZD 093522.50+395747.7
09354+3958 STF1369 AB 2009 40 149 25.2 6.98 7.98 NZD 093522.50+395747.7
09354+3958 STF1369 AB 2010 41 149 25.0 6.98 7.98 NZDV 093522.50+395747.7
09354+3958 STF1369 AB 2013 46 151 25.0 6.98 7.98 F2V NZDV 093522.50+395747.7
09354+3958 STF1369 AB 2015 51 149 24.9 6.98 7.98 F2V NZ V 093522.50+395747.7
09354+3958 STF1369 AB 2016 54 150 24.9 6.98 7.98 F2V NZ V 093522.50+395747.7
09354+3958 STF1369 AB 2017 57 149 25.0 6.98 7.98 F2V NZ V 093522.50+395747.7
09354+3958 STF1369 AB 2018 57 150 25.0 6.98 7.98 F2V NZ V 093522.50+395747.7
09354+3958 STF1369 AB 2019 59 150 25.1 6.98 7.98 F2V NZ V 093522.50+395747.7

If you need more information about this double, apply for a data request form to the WDS.