Details are in magnitude data page . The star is fainter than the plotted magnitude. Details are in magnitude data page . I-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, 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.