V787 Mon observation by Toa Akira Takao (Kita-kyushu, Japan) reports the discovery of large-amplitude variation in V787 Mon. From the amplitude in unfiltered CCD photometry, the object is more likely a Mira-type variable. V787 Mon = 2MASS 072000.852 -020906.34 (2000.0) 6.986 5.477 0.000 = IRAS07174-0203 071729.0 -020327 (1950.0) F12=5.25 F25=1.74 F60=0.40 F100=1.00L VAR=13 LRS=-1 VII: variable star with more evolved C-rich circumstellar shell = 072000.7 -020905 (2000.0) CGCS_J0720-0209 (CGCS1654) - 13.5 10.4 - = 072000.0 -020900 (2000.0) C(Buscombe) V=13.5 - - = 072000.3 -020904 (2000.0) IRAS07174-0203 5.165 1.669 0.405 1.012L 13% = 072000.3 -020904 (2000.0) SSC07174-0203 5.165 1.669 0.405 1.012L = 072000.7 -020905 (2000.0) CS1654 - 13.5 10.4 - CCD magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code MONV787 20010202.531 147C Toa.VSOLJ MONV787 20020111.685 145C Toa.VSOLJ MONV787 20020922.836 124C Toa.VSOLJ MONV787 20021122.636 122C Toa.VSOLJ MONV787 20030115.581 127C Toa.VSOLJ mag compared to GSC4820.662 Observer's code: Toa: Akira Takao (Kita-kyushu, Japan) instruments:f200mm F4 Telephotolens+ST-8,unfiltered Relayed from Akira Takao <drtakao@bronze.ocn.ne.jp>