Details are in magnitude data page . It was observed many times by the ASAS project. It is a Mira type variable star with a period of 390 days. John Greaves, UK, identified MisV0270 and ASAS 165942-2250.2. I I-band CCD magnitude observed by the ASAS project.
Details are in magnitude data page .
The ASAS observations reveal that it is SR-type with a period of 340 days. But the light curve behaves a bit strange around the peak. John Greaves, UK, identified MisV0271 and ASAS 170149-2301.3. Details are in magnitude data page . I-band CCD magnitude observed by the TASS project, researched by Michael Richmond.