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Table 4

Occurrence of the Hα third emission of RR Lyr around the pulsation phase, φ3Max, observed with ELODIE between 1994 and 1997.

Night ψ S/N φ3start φ3end φ3Max V3Max I3Max Vshock
(yyyy-mm-dd) (km s−1) (%) (km s−1)
1994-07-28 0.29 8 1.183 1.372 1.216 43 11
1994-07-29 0.31 7 1.194 1.252 1.240 41 11
1994-08-05 0.49 10 1.200 1.453 1.375 40 9
1995-09-05 1.60 7 1.219 1.375 1.282 44 14
1996-06-24 0.12 10 1.157 1.221 1.210 34 11 122
1996-06-26 0.18 9 1.306 1.373 1.317 33 11
1996-07-31 1.07 10 1.154 1.353 1.252 40 10
1996-08-01 1.10 9 1.157 1.306 1.306 41 10 143
1996-08-09 1.30 9 1.173 1.348 1.267 37 9
1996-08-25 1.71 10 1.238 1.408 1.335 44 11
1996-08-27 1.76 8 1.195 1.213 1.213 37 7
1997-08-05 2.66 7 1.192 1.326 1.299 40 8 139
1997-08-07 2.72 10 1.304 1.391 1.347 39 9
1997-08-08 2.74 9 1.196 1.395 1.299 37 7
1997-08-09 2.76 7 1.263 1.363 1.334 37 9 149
1997-08-29 3.28 12 1.181 1.350 1.243 44 9
1997-08-30 3.30 10 1.217 1.317 1.272 46 9 124
1997-08-31 3.33 5 1.153 1.197 (1.197) 42 8 121

Notes. Columns provide the date of the night, the corresponding Blazhko phase ψ, the pulsation phases at the beginning and at the end of the emission and at its maximum intensity. For this latter, the corresponding blueshifted velocity (km s−1) and the intensity of the Hα third emission with respect to the continuum are V3Max and I3Max, respectively. The last column gives the shock velocity Vshock (km s−1).

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