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Table 4.

Red and blue evolutionary modes for the LTVs of HR 8752, ρ Cas, and HD 179821 listed in chronological order.

Star Mode Trend Dates JD− Duration
of (B − V) 24 00000 (d)
HR 8752 Bpg-d 1899–1923 15000-23600 8600
Bpg-u 1923–2001 23600-52000 28400
V-uu B-u red 1942–1950 30500–33500 3000
V-d B-d const 1950–1957 33500–36000 2509
V-d B-d red 1957–1976 36000–43000 7000
V-d B-u blue 1976–2005 43000–53500 10500

ρ Cas V-u B-d red 1965–1982 34000–45000 6000
V-d B-dd red 1982–1986 45000–46500 1500
V-u B-uu blue 1986–1991 46500–48500 2000
V-c B-d red 1991–1998 48500–51000 2500
V-d B-dd red 1998–2000 51000–51300 300
V-c B-uu blue 2001–2009 52000–55500 3500
V-c B-dd red 2009–2013 55000–56500 1500
V-c B-u blue 2013–2015 56500–58100 1600

HD 179821 V-d B-u blue 1990–1993 48000–49200 1200
V-dd B-uu blue 1993–2004 49200–53200 4000
V-c B-d red 2004–2008 53200–54500 1300

Notes. Second column: u = up = brightness increasing, d = down = brightness declining, if double, i.e. uu and dd, the increasing and declining, respectively, are stronger than in the other channel, c = constant. Third column: const. = constant. For clarity, the trends “blue” are in boldface. For HR 8752 and ρ Cas, the transition from a red to a blue trend is caused by an eruption (1973, and 1986, 2000, 2013, respectively). Such a significant event for HD 179821 should have happened, but was obviously missed.

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