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\IBVShead{4842}{31 January 2000}

\IBVStitletl{New Variable Stars Discovered in the MISAO Project}{ VII: M\lowercase{is}V0351--M\lowercase{is}V0400 }

\IBVSauth{Yoshida, S.$^1$; Kadota, K.$^2$; Kato, T.$^3$}

\IBVSinst{MISAO Project, 1065-16 Miyawada Fujishiro-machi Kitasoma-gun, Ibaraki 300-1514, Japan,\\ \indent e-mail: seiichi@muraoka.info.waseda.ac.jp}
\IBVSinst{MISAO Project, 77-1-3-12-204 Koshikiya Ageo City, Saitama 362-0064, Japan,\\ \indent e-mail: kenic-k@astroarts.co.jp}
\IBVSinst{Dept.\ of Astronomy, Kyoto University, Kyoto 606-8502, Japan, e-mail: tkato@kusastro.kyoto-u.ac.jp}

\IBVSabs{This report describes 50 new variable stars (MisV0351-MisV0400)}
\IBVSabs{discovered in the course of the MISAO Project.}

\begintext

This report describes 50 new variable stars (MisV0351--MisV0400) discovered in the course of the MISAO Project.

These objects are detected automatically by the PIXY system as candidates of variable stars from unfiltered CCD images taken by Kadota between 1999 April and August, then confirmed by Yoshida and Kadota. Further details are the same as described in Yoshida and Kadota (1999).

Table 1 lists the 50 new variable stars. The position and magnitude are measured using the USNO-A1.0 catalog. The magnitude is based on a preliminary $V$ magnitude calculated from $R$ and $B$ magnitude in the catalog based on Kato's (1998) equation:
\[
V = R + 0.375 (B - R).
\]
The finding charts are available electronically as 4842-f$[nnn]$.eps, where $[nnn]$ refers to the serial number assigned to the star in the first column of Table~1.

MisV0360 is identified with a carbon star CS4603.

MisV0372 is within the positional error range of an X-ray source 1RXPJ180245-2942.3 at R.A. 18\hr02\mm45\fsec6, Decl.\ $-$29\deg42\arcm20\arcs\ (2000.0).

V2084 Sgr is 3.7 arcmin from MisV0391, that was detected on Kadota's unfiltered CCD images as another variable star between 9.8 and 10.8 mag. Therefore, MisV0391 is another new variable star.

NSV 12730 is 2.8 arcmin from MisV0393, that was detected as another variable star between 11.2 and 12.0 mag. Therefore, MisV0393 is another new variable star.

The photometry of MisV0395 was obtained as NGC 6194 No.\ 1130, which shows it is a red star (Mermilliod et al.\ 1994).

\vfil

\references

Kato, T., 1998, \\ {\tt http://www.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg00700.html}

Mermilliod, J.-C., Mermilliod, M., 1994, {\it Catalogue of Mean UBV Data on Stars}, Springer-Verlag

Yoshida, S., Kadota, K., 1999, {\it IBVS}, No.\ 4746

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\begin{table}
\begin{center}
\caption{List of New Variable Stars}
\begin{tabular}{crrrrcl} \hline
& & & \multicolumn{2}{c}{Unfiltered} \\
Code & \multicolumn{2}{c}{R.A. (J2000.0) Decl.} & \multicolumn{2}{c}{CCD Mag.} & Type & Identified with \\ 
& & & Max & Min \\
\hline
MisV0351 & 19\hr00\mm53\fsec82 & +00\deg06\arcm24\farcs0 & 12.5 & 14.3 & ? & USNO-A2.0 0900.13750040 \\
MisV0352 & 19 02 04.41 & +00 15 42.7 & 13.0 & 14.6 & ? & \\
MisV0353 & 19 57 35.03 & +37 14 50.6 & 12.6 & [14.8 & M? & USNO-A2.0 1200.13953227 \\
MisV0354 & 19 58 32.16 & +36 49 40.0 & 12.9 & [14.8 & SR? & \\
MisV0355 & 19 58 41.95 & +29 56 07.6 & 12.8 & 14.1 & ? & \\
MisV0356 & 19 58 55.32 & +11 07 03.3 & 12.0 & 12.9 & SR? & GSC 1075.0782 \\
MisV0357 & 19 59 13.95 & +15 30 44.7 & 12.9 & 13.7 & ? & USNO-A2.0 1050.15923840 \\
MisV0358 & 20 00 26.70 & +33 55 11.3 & 13.2 & 14.9 & ? & \\
MisV0359 & 20 00 32.83 & +13 13 28.0 & 12.9 & 13.8 & ? & USNO-A2.0 0975.17499216 \\
MisV0360 & 20 00 37.57 & +32 05 42.1 & 12.0 & 12.9 & SR? & CS4603 \\
MisV0361 & 20 01 05.88 & +22 01 58.6 & 12.9 & 14.6 & ? & USNO-A2.0 1050.16056563 \\
MisV0362 & 21 00 50.95 & +40 30 41.2 & 13.1 & 14.8 & ? & \\
MisV0363 & 22 04 39.25 & +53 35 29.7 & 12.7 & 14.0 & SR? & USNO-A2.0 1425.12761422 \\
MisV0364 & 22 03 05.68 & +42 44 07.6 & 10.5 & 11.8 & SR? & USNO-A2.0 1275.16948498 \\
\multicolumn{6}{c}{} & IRAS 22010+4229 \\
MisV0365 & 16 57 22.34 & $-$16 24 08.3 & 13.2 & 15.2 & ? & \\
MisV0366 & 20 56 10.02 & +46 34 53.0 & 13.1 & 14.9 & ? & \\
MisV0367 & 21 58 33.33 & +50 34 52.1 & 12.3 & 13.3 & SR? & USNO-A2.0 1350.15460187 \\
MisV0368 & 21 58 56.65 & +55 13 36.5 & 12.6 & 13.4 & SR & USNO-A2.0 1425.12612175 \\
MisV0369 & 19 00 11.85 & $-$02 57 24.4 & 10.8 & 13.6 & SR? & IRAS 18575-0301 \\
MisV0370 & 19 01 05.00 & $-$03 10 48.7 & 11.0 & 13.2 & SR? & IRAS 18584-0315 \\
MisV0371 & 18 57 32.71 & $-$18 55 17.2 & 13.8 & 15.2 & SR? & \\
MisV0372 & 18 02 43.69 & $-$29 42 14.8 & 11.9 & [14.4 & M? & \\
MisV0373 & 20 57 09.29 & +35 18 44.2 & 11.0 & 12.7 & ? & GSC 2696.3197 \\
\multicolumn{6}{c}{} & USNO-A2.0 1200.16576581 \\
\multicolumn{6}{c}{} & IRAS 20552+3507 \\
MisV0374 & 21 02 34.30 & +38 12 33.2 & 12.9 & 14.1 & ? & USNO-A2.0 1275.14555028 \\
MisV0375 & 16 59 59.33 & $-$09 33 01.0 & 13.0 & [15.0 & SR? & \\
\hline
\end{tabular}
\end{center}
\end{table}

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\addtocounter{table}{-1}
\begin{table}
\begin{center}
\caption{cont.}
\begin{tabular}{crrrrcl} \hline
& & & \multicolumn{2}{c}{Unfiltered} \\
Code & \multicolumn{2}{c}{R.A. (J2000.0) Decl.} & \multicolumn{2}{c}{CCD Mag.} & Type & Identified with \\ 
& & & Max & Min \\
\hline
MisV0376 & 17 57 31.45 & $-$15 38 16.3 & 13.3 & [14.4 & ? & USNO-A2.0 0675.23576359 \\
\multicolumn{6}{c}{} & IRAS 17546-1537 \\
MisV0377 & 17 58 11.26 & $-$17 25 42.9 & 13.0 & [14.3 & ? & IRAS 17553-1725 \\
MisV0378 & 17 58 12.45 & $-$13 40 42.1 & 13.1 & [14.5 & ? & IRAS 17553-1340 \\
MisV0379 & 17 58 54.36 & $-$14 51 52.8 & 12.2 & [14.6 & M? & USNO-A2.0 0750.12439396 \\
MisV0380 & 17 59 05.61 & $-$16 55 33.0 & 12.8 & [14.4 & ? & \\
MisV0381 & 17\hr59\mm15\fsec91 & $-$12\deg07\arcm17\farcs7 & 13.2 & 14.4 & SR? & USNO-A2.0 0750.12451923 \\
MisV0382 & 17 59 36.49 & $-$16 19 33.8 & 12.1 & [14.5 & ? & \\
MisV0383 & 17 59 38.83 & $-$15 57 57.9 & 12.9 & 14.4 & SR? & \\
MisV0384 & 18 00 49.76 & $-$16 12 54.4 & 13.0 & [14.5 & ? & USNO-A2.0 0675.23803931 \\
MisV0385 & 18 00 55.03 & $-$14 38 28.6 & 12.3 & 14.2 & SR? & \\
MisV0386 & 18 01 25.89 & $-$14 56 30.8 & 13.2 & [14.6 & SR? & USNO-A2.0 0750.12524613 \\
MisV0387 & 18 02 06.82 & $-$16 24 44.9 & 12.5 & [14.4 & ? & USNO-A2.0 0675.23888438 \\
\multicolumn{6}{c}{} & IRAS 17592-1625 \\
MisV0388 & 18 02 11.87 & $-$11 40 01.7 & 11.4 & 13.6 & ? & IRAS 17593-1140 \\
MisV0389 & 18 30 44.94 & +03 45 22.2 & 11.1 & 12.1 & ? & USNO-A2.0 0900.13032893 \\
\multicolumn{6}{c}{} & IRAS 18282+0343 \\
MisV0390 & 18 58 59.01 & $-$15 48 10.5 & 13.1 & 15.3 & ? & USNO-A2.0 0675.30915787 \\
MisV0391 & 18 59 27.21 & $-$13 51 22.9 & 13.2 & 14.5 & SR? & IRAS 18565-1355 \\
MisV0392 & 19 58 06.32 & +36 59 09.9 & 12.6 & [15.0 & M? & \\
MisV0393 & 20 02 20.39 & +37 18 01.1 & 13.1 & 14.6 & SR? & USNO-A2.0 1200.14247813 \\
MisV0394 & 17 00 52.60 & $-$02 28 35.2 & 12.6 & 13.9 & ? & USNO-A2.0 0825.09947996 \\
\multicolumn{6}{c}{} & IRAS 16582-0224 \\
MisV0395 & 17 56 57.17 & $-$18 52 12.6 & 13.2 & [14.2 & ? & IRAS 17540-1851 \\
MisV0396 & 17 57 01.97 & $-$14 23 09.7 & 11.6 & 12.8 & SR? & USNO-A2.0 0750.12377050 \\
\multicolumn{6}{c}{} & IRAS 17541-1422 \\
MisV0397 & 17 57 42.00 & $-$20 13 38.5 & 13.1 & 14.2 & ? & IRAS 17547-2013 \\
MisV0398 & 17 57 48.50 & $-$17 30 34.7 & 12.5 & 16.3 & ? & IRAS 17548-1730 \\
MisV0399 & 17 57 46.44 & $-$10 53 53.6 & 12.3 & [14.7 & M? & IRAS 17550-1053 \\
MisV0400 & 17 57 49.35 & $-$13 34 05.3 & 12.9 & 14.0 & ? & IRAS 17550-1333 \\
\hline
\end{tabular}
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\end{table}

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