A. M. van Genderen, A. Jones and C. Sterken
We present time-series monitoring of 19 Magellanic Cloud super- and hypergiants, of which 6 turned out to be constant, and 13 are alpha Cygni variables, viz.: S18 = AzV154, HDE268835 = R66, HD37974 = R126, HDE268757 = R59, HDE268822 = GV505, HDE269355 = GV258, HDE269612 = GV322, HDE270025 = GV439, AzV121, HD5277 = AzV136 = R10, AzV197, AzV310 = R26, and AzV369; the LMC stars HD32034 = GV80 = R62, HDE268819 = GV91, HDE269661 = GV346 = R111, HDE269697 = GV352, HDE269953 = GV423 = R150 and HDE270111 = GV460.
Manuscript in pdf format: jad12_4.pdf
| Table | Description |
| R59AFJ | Visual magnitude estimates of R59 |
| R66AFJ | Visual magnitude estimates of R66 |
| R126AFJ | Visual magnitude estimates of R126 |
| R66UVBY | uvby photometry of R66 in the instrumental system |
| S18 | Table 5: Walraven photometry of S18 |
| HD37974 | Table 6: Walraven photometry of HD37974 = R126 |
| HD268835 | Table 7: Walraven photometry of HDE268835 = R66 |
| HD268757 | Table 8: Walraven photometry of HDE268757 = R59 |
| HD269612 | Table 9: Walraven photometry of HDE269612 = GV322 |
| HD268822 | Table 10: Walraven photometry of HDE268822 = GV505 |
| AZV369 | Table 11: Walraven photometry of AzV369 |
| G91 | Table 12A: Walraven V photometry of G91 |
| G352 | Table 12B: Walraven V photometry of G352 |
| G423 | Table 12C: Walraven V photometry of G423 |
| HD270111 | Table 13: Walraven photometry of HDE270111 = G460 |
| G80 | Table 14A: Walraven V photometry of G80 |
| G346 | Table 14B: Walraven V photometry of G346 |