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(cba:news) CI Aquilae in particular (Joe Patterson) [2021-07-08T03:40:37Z]


Hi CBAers,

I just wanted to push CI Aquilae a little extra hard. As you know, it's a recurrent nova, and the only RN which can answer the question: is the great oddity of T Pyx/IM Nor (Mv, dP/dt) due to the short P_orb, or due to some other effect special to RNe (e.g. extreme and frequent heating of the donor). The really long-P_orb RNe are not appropriate for such a test, because giant stars will be heated much less strongly - i.e. their properties are probably determined by the whims of the donor, not any binary interaction.

It's an equatorial star well-placed for everyone. The only catch is that you absolutely need a long run - at least 5 hours if possible. P_orb = 15 hours, so define the orbital wave, you need some decent fraction of that. Maybe 4 hours is OK. That will often yield a pretty boring light curve... but with other longitudes pitching in, it'll be much better.

July-August is totally the season for novae! Southern guys of course, because of the rich pickings in Sco-Sgr... but also some in the north or equatorial (V1974 Cyg, V1494 Aql, CI Aql, others). As usual, it's best to pick a program star and beat on it faithfully for a few weeks. That's what makes these campaigns scientifically impactful.

joe
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