Following observations extracted from vsnet-obs reports seem to indicate ER UMa never faded to its quiescence in January. The light curve in late Januanry to early February looks like a standstill or an extended superoutburst accompanied by a brightening around Feb. 1. Previous superoutbursts of ER UMa usually last 19 days (with a very regular duty cycle ~0.4 to its supercycle 43 days). Has its outburst property changed? Please keep a close eye on this particuliar dwarf nova, the best known and the brightest member among its allies (ER UMa stars or RZ LMi stars -- cf. http://www.kusastro.kyoto-u.ac.jp/vsnet/DNe/eruma.html).
YYMMDD(UT) mag code 970101.051 133 POY 970101.938 135 POY 970103.051 138 POY 970103.892 125 JEN 970106.866 125 JEN 970107.869 124 PIE 970109.633 126 Wnt 970109.947 131 JEN 970111.849 130 PIE 970111.948 130 JEN 970112.605 13.27V Oud 970113.594 13.25V Oud 970113.840 132 PIE 970114.900 132 PIE 970114.965 135 POY 970114.994 127 JEN 970115.633 13.43V Oud 970115.869 131 PIE 970116.830 133 PIE 970117.783 136 Wnt 970117.901 135 POY 970117.926 138 JEN 970119.871 13.55V Oud 970125.842 137 POY 970126.792 135 BMU 970126.817 137 POY 970128.849 135 POY 970131.773 132 Wnt 970201.780 130 PIE 970201.797 135 JEN 970201.823 13.35V Oud 970201.887 135 BMU 970202.917 135 POY 970203.646 135 Wnt 970205.960 142 PIE 970206.860 151: PIE 970207.860 148 POY
Regards,
Taichi Kato
ER UMa
Observations reported to vsnet-obs indicate the superoutburst is apparently
overdue since its last in January. This may be somehow associated with the
possible unexpected duration of the January superoutburst (cf. vsnet-alert
718, http://www.kusastro.kyoto-u.ac.jp/vsnet/DNe/erumaob.html).
Observers are strongly urged to monitor closely this ER UMa-type prototype
to see if any change of supercycle (formerly length = 43 days) happens.
Return to Powerful Manager's page
ER UMa: superoutburst overdue
YYMMDD(UT) mag code
970125.842 137 POY
970126.792 135 BMU
970126.817 137 POY
970128.135 13.52 JEN
970128.849 135 POY
970131.773 132 Wnt
970201.780 130 PIE
970201.797 135 JEN
970201.823 13.35V Oud
970201.887 135 BMU
970202.917 135 POY
970203.646 135 Wnt
970205.960 142 PIE
970206.860 151: PIE
970207.860 148 POY
970209.812 139 Wnt
970211.156 149 POY
970211.648 <139 Wnt
970213.817 142 POY
970218.701 <134 Wnt
970218.869 <141 POY
970219.607 <134 Wnt
970221.715 <130 Wnt
970221.822 132 POY
Regards,
Taichi Kato
vsnet-adm@kusastro.kyoto-u.ac.jp