\documentstyle[epsf,twoside]{article}

\input ibvs2.sty
\input ibvst.sty

\begin{document}

\IBVShead{4735}{13 July 1999}

\IBVStitle{Discovery of a New Mira Variable}

\IBVSauth{P.K. Abolmasov$^1$, S.Yu. Shugarov$^2$}

\IBVSinst{Moscow City Palace for Youth's Creativity, 17, Kosygina Str., Moscow 117978, Russia}

\IBVSinst{Sternberg Astronomical Institute, 13, Universitetskij Av., Moscow 119899, Russia,\\ e-mail: shugarov@sai.msu.ru}

\SIMBADobj{IRAS 17506+3411}

\begintext

\IBVSTnam{IRAS 17506+3411 = USNO A1.0 1200.08799479}

\IBVSTcoo{17\hr52\mm24\fsec1}{+34\deg11\arcm12\arcs}{J2000.0}

\IBVSTobs{40-cm astrograph in Crimea}

\IBVSTdet{Photoplate}

\IBVSTfil{None}

\IBVSTcomp{See Fig.~1}

\IBVSTchk{None}

\IBVSTsys{$B_{pg}$}{$B$-band standard sequence in SA 62 (Prieser, 1974)}

\IBVSTdata{Upon request}

\IBVSTtyp{ M }

\IBVSTrem{
The variability of the star was discovered by S. Antipin (priv.\ comm.). 160 estimates in interval JD2433031--49634 show variations typical of Mira type variable with the following light elements: 
$$
{\rm JD_{max}} = 2445197 + 261\fday3 \times E.
$$ 
The range of variability is 13\fmm8--17\fmm5.}

\IBVSTack{The authors would like to thank Dr.\ V.P. Goranskij for his help and useful discussion.}

\newpage

\IBVSfig{7.5cm}{4735-f1.ps}{Finding chart and comparison stars.}

\IBVSfig{7.5cm}{4735-f2.ps}{Phased light curve. Uncertain estimates are shown as open circles, ``v'' symbols represent upper limits.}

\reference

Prieser, J.B. 1974, Naval Observ.\ Publ., vol.\ XX, p.\ VII, Washington

\end{document}

