NSV25735 = StHA190 According to astro-ph/0102192, Munari et al. repoorts the discovery of bipolar and highly variable mass outflow in NSV25735 = StHA190. Such phenomena have been notably known in R Aqr, CH Cyg, MWC 560 = V694 Mon, RS Oph and Hen3-1341. NSV25735 = StHA190 is the first case that a yellow symbiotic hosts such outflows. Since this object is very bright, detailed observations are strongly encouraged. Identifications: GSC547.712 214144.86 +024354.5 (2000.0) 11.16 0 GSC547.712 214144.90 +024354.4 (2000.0) 10.84 1 USNO0900.19923635 214144.870 +024354.13 (2000.0) 11.0 12.1 * IRAS21392+0230 213912.4 +023011 (1950.0) F12=1.90 F25=1.58 F60=0.40L F100=3.02L VAR= 0 LRS=-1 possibly IIIa: variable star with more evolved O-rich c.s. shell 214144.7 +024354 (2000.0) StHA190 10.5 - ZAND 214144.3 +024352 (2000.0) IRAS21392+0230 1.844 1.647 0.400L 2.953L 0% 214144.3 +024352 (2000.0) SSC21392+0230 1.844 1.647 0.400L 2.953L 214144.4 +024352 (2000.0) FSC21392+0230 1.796 1.635 0.221 3.273L 214144.7 +024352 (2000.0) Ste190 10.5v ZAND 214144.9 +024359 (2000.0) RJ120 10.1V 214144.8 +024354 (2000.0) 1030 0.84 TYC547.712.1 plx=34.9(37.3) (0.07 0.09) 214144.8 +024353 (2000.0) 1023 0.88 TYC2-547.712.1 (10.32 0.05) (11.36 0.09) 214144.3 +024352 (2000.0) NSV25735 ZAND: 7.75 7.89 K pec(e) According to T. Watanabe, the object has been photometrically highly variable. Observations reported to VSNET follow: YYYYMMDD(UT) mag observer 19941006.560 110 (M. Moriyama) 19951115.566 107 (M. Moriyama) 19960922.688 107 (T. Watanabe) 19961011.657 107 (T. Watanabe) 19961115.548 106 (T. Watanabe) 19961130.510 108 (T. Watanabe) 19970908.710 105 (M. Moriyama) 19971001.619 113 (T. Watanabe) 19971027.535 107 (T. Watanabe) 19971204.515 115 (T. Watanabe) 19980105.449 111 (T. Watanabe) 19980822.732 114 (T. Watanabe) 19980903.626 108 (T. Watanabe) 19981107.556 112 (T. Watanabe) 19991225.421 111 (T. Watanabe) Regards, VSNET Collaboration team