NNo GCVS J2000.0 Type Max Min I Min II Epoch Year Period M-m/D Spectrum References Other desig. p.m.(as/yr) Epoch Ident. New type GCVS
--------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
731708 |V1708 Sco *|172341.94 -310307.6 |NC:+SR | 13.2 | 18.2 | |V |59102. |2020 | | |pec(Nova) |82238 2MASS| |-0.002 -0.010|2000.0 | |Gaia DR2 |NSim:+SR |V1708 Sco |
--------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
_______________Cross-identifications:_______________
V1708 Sco = 2MASS J17234193-3103075 |
V1708 Sco = Nova Sco 2020 |
V1708 Sco = TCP J17234205-3103072 |
____________________________________________________
Reference to a chart or photograph:
2MASS Skrutskie M.F., Schneider S.E., Stiening R., Strom S.E., Weinberg M.D., Beichman C., Chester T., Cutri R., Lonsdale C., Elias J., Elston R., Capps R., Carpenter J., Huchra J., Liebert J., Monet D., Price S., Seitzer P., The Two Micron All Sky Survey, 2nd Intermediate Data Release, Proc. Workshop "The Impact of Large Scale Near-IR Sky Surveys", 25 (1997) (CDS Cat. II/246).
Reference to a study of the star:
82238. http://meineko.sakura.ne.jp/ccd/PNV_J17561375-2942546.jpg
__________________________________________________________________
Remark:
According to [240], the star showed semiregular variations before its outburst with a peak-to-peak amptitude about 1m and P = 140.5d.
----The End----