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Ok, I understand, Olivier,
but nevertheless, could you be so kind to pass them my posting?

Ernst

Hi Olivier, you write in capter 4.3.1: In short, despite our ability to reproduce fairly well the Hα line profile of P Cygni observed in 2020 using such a less intense wind model, it is beyond the scope of the current paper to state that the intensity of the wind of P Cygni varied in this way during...

Hi Olivier, would you be so kind to send a copy of the paper? Another question: what about the evaluation of the del Sco spectra at BeSS? Are there further not jet evaluated spectra of other observers? Because of the periastron passage radial velocity of the star as much spectra as possible would be...

Dear colleagues, Halpha radial velocity measurements of delta Sco are urgend required to determine the exact periastron time and to clarify the enigmatic RV dip linked with the question of a third body within that system. As it is seen, this RV dip have been first time observed during the campaign 2...

The very successfuly spectroscopy conference VEGA22 took place in Salzburg (Austria). The following link allows to watch some of the talks of that conderence. The other talks will be provide next days.
https://www.astrophoto.at/VEGA/vega-2022.html

Ernst Pollmann

Dear Joan,
the Halpha spectrum would be very helpful to determine the radial velocity during the periastron passage, the campaign of Anatoly Miroshnichenko.
Please send me your spectrum for evaluation of this parameter.

Ernst

... at the AAVSO data base:

https://app.aavso.org/avspec/search

Ernst

Hi Joan, I think there are a lot of other colleagues here within this forum, who could give also interesting and helpful inputs concerning your posting above. As you know, the field of my activity is constraint more on medium and high resolution spectroscopy, then within the low resolution field. I ...

The Spectroscopy Magazine BAVMS will be available now at:
https://ui.adsabs.harvard.edu/search/q= ... 0desc&p_=0

Ernst Pollmann

Dear colleagues,
the descent of the Halpha radial velocity does have started.
Please take spectra of the star for determination of the periastron time.
Ernst Pollmann