\documentstyle[twoside,epsf]{article}

\input ibvs2.sty
\input ibvst.sty

\begin{document}

\IBVShead{4615}{27 July 1998}

\IBVStitle{New Outbursts of V1118 O\lowercase{ri}}

\IBVSauth{Tomonori HAYAKAWA, Takuma UEDA, Makoto UEMURA, Hiroyuki OHASHI, Taichi KATO, Katsura MATSUMOTO }


\IBVSinst{Dept.\ Astron., Faculty of Sci., Kyoto University, Sakyo-ku,
Kyoto 606-01, Japan }

\begintext


\IBVSTnam{V1118 Ori}

\IBVSTcoo{05\hr 34\mm 44\fsec 2
}{$-$05\deg 33\arcm 40\arcs
}{2000
}

\IBVSTobs{Ouda observatory in Nara with 60cm telescope
}

\IBVSTdet{CCD
}

\IBVSTfil{V
}

\IBVSTcomp{GSC4774.826
}

\IBVSTchk{GSC4774.878
}

\IBVSTsysn

\IBVSTrem{Since 1983, when V1118 Ori became known as a new EXor
(Herbig, 1990, refers to this species as EXor, after the example first
recognized, EX Lupi or Subfuor, Parsamian and Gasparian, 1987) and
entered into an active stage of fuor-like outburst, three outbursts
have been observed.  As of now we have information concerning outbursts
during the period 1983-84 (Chanal, 1983, Parsamian and Gasparian,
1987), 1988-90, and 1992-93 (Parsamian et al., 1993). And now, we
observed a new outburst of V1118 Ori in 1997.}

\references

Chanal, M., 1983, IAUC, No.\,3763

Herbig G. H., 1990, Low Mass Star Formation and Pre-Main Sequence
Objects, ed.\ Bo Reipurth, M\"{u}nchen, 233

Parsamian, E.S. and Gasparian, K.G., 1987, Astrofizika, 27, 447

Parsamian, E.S., Ibragimov, M.A., Ohanian, G.B. and Gasparian, K.G., 1993,
Astrofizika, 36, 23

\endreferences

\IBVSfig{10cm}{4615-f1.ps}{The field of V1118 Ori. (The size of the
field is $7\arcm \times 10\arcm$ and north is top.)}

\IBVSfig{10cm}{4615-f2.ps}{The light curve of V1118 Ori.}

\end{document}
