I-band CCD magnitude observed by the TASS project, researched by Michael Richmond. V V-band CCD magnitude observed by the TASS project, researched by Michael Richmond. It may be a Mira type variable star with a rough period of 300-400 days. Details are in magnitude data page . I-band CCD magnitude observed by the TASS project, researched by Michael Richmond.
Details are in magnitude data page .
I-band CCD magnitude observed by the TASS project. I-band CCD magnitude observed by the ASAS project. 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.