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comet and spectroscopi observations on 17 march

after a sunny day, we also got a clear night with low temperatures around freezing. Transparency was initially reasonable with SQM in zenith of 18.7 to go to 19.2 later in the evening/night and drop back as the moon came out. Comets that could be observed with my 0.4-m f/3.8 Newtonion telescope were: 29P, 496P, P/2019 Y3, C/2022 E2, C/2023 H5, C/2023 Q1, C/2025 D1 (not detected in background of magn. 20.3). With the 2nd observatory ( 0.28-m f/10 cassegrain telescope with LHiReSS-III spectrograph), high resolution spectra of H-alpha region were recorded from PZ Gem (esxposure: 8 x 1200 sec) and 4 Her (exposure: 3 x 1200 sec)

manuscript “The birth of Be star disks… ” published

The paper made by Jonathan Labadie-Bartz was today published: “The birth of Be star disks I. from localized ejection to circularization”; abstract:

Classical Be stars are well known to eject mass to build up a disk, but the details governing the initial distribution and subsequent evolution of this matter into a disk are in general poorly constrained through observations.
Aims. By combining high-cadence time-series spectroscopy with contemporaneous space photometry from the Transiting Exoplanet Survey Satellite (TESS), we have sampled about 30 mass ejection events in 13 Be stars. Our goal is to constrain the geometrical and kinematic properties of the ejecta as early as possible

comet and spectroscopic observations on 5 march

the clear sky is perfect to observe some comets: comets that could be observed are: 29P, 43P, 49P, 476P, C/2022 E2, C/2023 H5, C/2024 A1, P/2023 S1. With my second setup, i could obtain spectra in H-alpha region of Be-stars : gam Cas, PZ Gem and Phecda

comet and spectroscopic observations on 3 march 2025

After a beautiful sunny day, it was also a clear night, though with a bit less transparency. I was able to observe several comets until high clouds are drift in. Still a number of comets were observed such as: 29P, 43P, 276P, 472P, 487P, 496P, A/2025 A7, C/2017 K2, P/2019 Y3. Simultaneously, with the 2nd observatory, spectra were obtained in high resolution (R~15000) in H-alpha region of the Be stars: gam Cas, PZ Gem and 53 Boo.