120 Minima timings of eclipsing binaries

We present 120 times of minima of 8 eclipsing binaries

Percutaneous Catheter Dilatation of Benign Ureteroenteric Anastomotic Strictures Followed or not by Retrograde Transconduit Placement of a Catheter: Long Term Results

BACKGROUND: We report our experience on multiple balloon dilatations for benign ureteroenteric anastomotic strictures after total cystectomy and urinal deviation by ileal conduit, followed or not by retrograde placement of a permanent catheter through the stoma of the ileal conduit. PATIENTS AND METHODS: Patients were classified in two groups: Group A included patients treated only by multiple balloon dilatations and Group B patients in whom multiple dilatations were followed by retrograde insertion of a permanent catheter through the stoma of the ileal conduit, which then had to be replaced regularly. Records of survival and patency rates were recorded. RESULTS: Twenty patients with 24 benign ureteroenteric anastomotic strictures referred to radiology department. Long-term results were available in only 15 patients, who finally included in the study. In Group A long term follow-up was achieved in five patients. Mean primary patency time of stenoses (interval between initial dilatation and recurrence) was 33.2 months. This time-period proved to be the same as the survival time of Group A patients, since all five patients eventually succumbed to the underlying disease or other reasons. In Group B, 6 patients are still alive and 4 patients eventually succumbed to the underlying disease or other reasons. Mean primary patency time of stenoses was 38.1 months. CONCLUSIONS: Balloon dilatations of benign ureteroenteric anastomotic strictures, due to radical cystectomy and urinal deviation by ileal conduit, were technically successful in all cases. Patency rate was comparable in the two study groups. However, regular catheter replacement through the ileal conduit is well tolerated and gives a sense of security to both patient and physician

CzeV1731: The unique doubly eclipsing quadruple system

We report the discovery of the relatively bright (V = 10.5 mag), doubly eclipsing 2+2 quadruple system CzeV1731. This is the third known system of its kind, in which the masses are determined for all four stars and both the inner and outer orbits are characterized. The inner eclipsing binaries are well-detached systems moving on circular orbits: pair A with period PA = 4.10843 d and pair B with PB = 4.67552 d. The inner binaries contain very similar components (q  ≈  1.0), making the whole system a so-called double twin. The stars in pair B have slightly larger luminosities and masses and pair A shows deeper eclipses. All four components are main-sequence stars of F/G spectral type. The mutual orbit of the two pairs around the system barycenter has a period of about 34 yr and an eccentricity of about 0.38. However, further observations are needed to reveal the overall architecture of the whole system, including the mutual inclinations of all orbits. This is a promising target for interferometry to detect the double at about 59 mas and ΔMbol <  1 mag

The PHEMU21 catalogue and astrometric results of the observations of the mutual occultations and eclipses of the Galilean satellites of Jupiter made in 2021

International audience2021 was the year of Jupiter's equinox, that is the Sun and the Earth passed through the equatorial plane of the planet and therefore the orbital planes of its main satellites. This occurrence made it possible to observe mutual occultations and eclipses between the satellites. Our former experience shows that observations of such events provide accurate astrometric data that can be used to obtain new information on the dynamics of the Galilean satellites. The observations are a series of photometric measurements of a satellite which are carried out through the organization of a world wide campaign of observations thus maximizing the number and the quality of the data obtained. This work focuses on processing the photometric observations of the mutual occultations and eclipses of the Galilean satellites of Jupiter made during the international campaign in 2021. The final goal is to derive new accurate astrometric data. We used an accurate photometric model of mutual events in conjunction with the accuracy of observation. We obtained and processed the 84 light curves obtained during the campaign. As compared with the current best ephemerides, the rms of 'O-C' residuals are equal to 49 and 48 mas in right ascension and declination, respectively