T Pyx

$B!!#T!!#P#y#x(B            NR             6.5-15.3p

$B!!(B1902$BG/$NA}8w$r(BLeavitt$B$,H/8+!#(B1890$BG/!"(B1902$BG/!"(B1920$BG/!"(B1944$BG/!"(B1966$BG/$KA}(B
$B8w$7$F$$$k!#A}8w$9$k$H$$$&1=$,$"$k$b$N$N$^$@$G$"$k!#(B12$BEyBf$^$GA}8w$7$?$H$$(B
$B$&>pJs$b$"$C$?$,5?$o$7$$!#:G6a$N4QB,$G$O#1#4!%#8#0#V!"%9%Z%/%H%k$K$O%P%k%^(B
$B!<51@~!"#H#e-6!\#C-7!"#H#e#I51@~$,G'$a$i$l$k!#FC$KB>$N#N#L$H0c$&=j$O$J$$!#(B

920630
$BO@J8>R2p!'#T!!#P#y#x$N50F;<~4|(B

  "The Photometric Period of the Recurrent Nova T Pyxidis"
  Ap. J. Sup. 81, vol 1 (1992)
  Bradley E. Schaefer, Arlo U. Landolt, Nikolaus Vogt, David Buckley,
  Brian Warner, Alistair R. Walker and Howard E. Bond

$B!!$^$@(BAbstract$B$7$+8+$F$$$J$$$N$G$9$,!">R2p$r!#(B
$B!!(BT Pyx$B$O?t>/$J$$H?I|?7@1$N0l$D$G!"$=$NCf$G$bFC$K!"DL>o$N?7@1$HF1$8$h$&$K(B
$BO"@1Cf$NGr?'bd@1I=LL$G$NG.3KH?1~$NK=Av$,GzH/5!9=$H9M$($i$l$F$$$k$b$N$G$9!#(B
$B!JB>$K$O(B U Sco, V394 CrA, Nova LMC 1990 No.2 $B$N#3@1$,$"$j$^$9!K(B
$B!!(B1986-1990$BG/$N#B%P%s%IB,8w(B1713$BE@$+$i!"#2;~4V$N%*!<%@!<$G(B0.09$BEy$NJQF0$,B8(B
$B:_$9$k$3$H$,L@$+$K$J$C$F$$$^$9$,!"?tF|0J>e$r$*$/$H0LAj$,B7$o$:!"@:L)$J<~4|(B
$B$O5a$a$i$l$J$$$N$@$=$&$G$9!#$=$l$G$b#1HU$N$&$A$N$=$N<~4|$NJQF0$OM-0U@-$,9b(B
$B$$$N$G!":G$b3N$+$i$7$$<~4|$r5a$a$F$_$k$H(B0.07737$B$^$?$O(B0.07616$BF|$H$J$C$?$=$&(B
$B$G$9!#6a!9?7@1GzH/$,4|BT$5$l$k$3$N@1$G!"GzH/$K$*$1$k50F;<~4|$NJQ2=$r8!=P$7(B
$B$F!"GzH/$K$*$1$kJ*