According to "Astronomical Time Series" (ed Maoz et al. 1997, Kluwer Academic Press) p.195, Tovmassian et al. identified the ROSAT source RX J0757.0+6306 (=1RXS J075700.5+630602) as a new, ultrashort-period cataclysmic variable. The orbital period is 75+/-1.4 min. The optical spectrum shows strong hydrogen emission lines, resembling that of WZ Sge. Tovmassian et al. discussed in this paper the possibility of a DQ Her type. This star may be worth monitoring for possible future outbursts. The paper did not mention the accurate coordinates, but watching at the ROSAT position (07h 57m 00s.5, +63o 06' 02" 2000.0) might be sufficient. Regards, Taichi Kato