Results 71 to 80 of about 7,595 (254)
Corrected μβ for stars of Hipparcos catalogue from independent latitude observations over many decades [PDF]
During the last century, there were many so-called independent latitude (IL) stations with the observations which were included into data of a few international organizations (like Bureau International de l'Heure - BIH, International Polar ...
Damljanović G., Milić I.S.
doaj +1 more source
COMMISSION 8: ASTROMETRY [PDF]
Gaia is continuing well with its development and construction and is expected to achieve parallax accuracies of about 10 to 300 muas for 6 to 20 mag. It is scheduled to launch in 2013.
Evans, Dafydd W.+9 more
openaire +2 more sources
The fireball of November 24, 1970, as the most probable source of the Ischgl meteorite
Abstract The discovery of the Ischgl meteorite unfolded in a captivating manner. In June 1976, a pristine meteorite stone weighing approximately 1 kg, fully covered with a fresh black fusion crust, was collected on a mountain road in the high‐altitude Alpine environment.
Maria Gritsevich+15 more
wiley +1 more source
Astrometry during the past 100 years [PDF]
The reports from 2008: "Astrometry and optics during the past 2000 years", are available at arXiv and at my website: www.astro.ku.dk/~erik/History.pdf . Here are now further contributions to the history of astrometry related to space astrometry. The development of photoelectric astrometry is followed from an experiment in 1925 up to the Hipparcos ...
arxiv
The Optical Wide-field patroL-Network (OWL-Net) is a global optical network for Space Situational Awareness in Korea. The primary operational goal of the OWL-Net is to track Low Earth Orbit (LEO) satellites operated by Korea and to monitor the ...
Jin Choi, Jung Hyun Jo, Sooyoung Kim
doaj +1 more source
Method for estimating the accuracy of astrometric (rectangular coordinates) and photometric (diameters and magnitudes) characteristics of commercial scanners is proposed and applied.
Yu. I. Protsyuk+10 more
doaj +1 more source
Gaia23ckh: Symbiotic outburst of the assumed Mira variable V390 Sco
Abstract The poorly studied variable star V390 Sco, previously classified as a Mira pulsator, was detected in a brightening event by the ESA Gaia satellite in September 2023. This work presents an analysis of available archival multifrequency photometric data of this target, along with our spectroscopic observations. Our findings lead to the conclusion
Jaroslav Merc+7 more
wiley +1 more source
Astrometry 1960-80: from Hamburg to Hipparcos [PDF]
Astrometry, the most ancient branch of astronomy, was facing extinction during much of the 20th century in the competition with astrophysics. The revival of astrometry came with the European astrometry satellite Hipparcos, approved by ESA in 1980 and launched 1989.
arxiv
Magnetic Field Studies in BL Lacertae through Faraday Rotation and a Novel Astrometric Technique
It is thought that dynamically important helical magnetic fields twisted by the differential rotation of the black hole’s accretion disk or ergosphere play an important role in the launching, acceleration, and collimation of active galactic nuclei (AGN ...
Sol N. Molina+3 more
doaj +1 more source
The deep eclipses of RW Aur revisited by long‐term photometric and spectroscopic monitoring
Abstract RW Aurigae is a young stellar system containing a classical T Tauri star as the primary component. It shows deep, irregular dimmings, first detected in 2010. At the University Observatory Jena, we carried out optical follow‐up observations. We performed multiband (BVRI) photometry of the system with the Cassegrain‐Teleskop‐Kamera II and the ...
Oliver Lux+2 more
wiley +1 more source