62 citations
- University of ViennaAT4 papers
- Comenius University BratislavaSK3 papers
- University of StuttgartDE2 papers
- California Institute of TechnologyUS1 paper
- Centre National de la Recherche ScientifiqueFR1 paper
- Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR)DE1 paper
- ETH ZurichCH1 paper
- European Space Astronomy CentreES1 paper
- GeoInformation (United Kingdom)GB1 paper
- Infrared Processing and Analysis CenterUS1 paper
- Institut de Mécanique Céleste et de Calcul des ÉphéméridesFR1 paper
- Institut de physique du globe de ParisFR1 paper
6 papers
Spectral properties of ablating meteorite samples for improved meteoroid composition diagnostics
Pavol Matlovič, Adriana Pisarčíková, Veronika Pazderová +7
Emission spectra and diagnostic spectral features of a diverse range of ablated meteorite samples with a known composition are presented. We aim to provide a reference spectral dat…
The new Herschel/PACS Point Source Catalogue
Gábor Marton, Ilknur Gezer, Máté Madarász +6
Herschel operated as an observatory, therefore it did not cover the whole sky, but still observed ~8% of it. The first version of an overall Herschel/PACS Point Source Catalogue wa…
The Fireball of November 24, 1970, as the Most Probable Source of the Ischgl Meteorite
Maria Gritsevich, Jarmo Moilanen, Jaakko Visuri +13
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 en…
Hydrogen emission from meteors and meteorites: mapping traces of HO molecules and organic compounds in small Solar system bodies
Pavol Matlovič, Adriana Pisarčíková, Juraj Tóth +8
The hydrogen emission from meteors is assumed to originate mainly from the meteoroid composition, making it a potential tracer of HO molecules and organic compounds. H lin…
Hydrodynamic escape of water vapor atmospheres near very active stars
Colin P. Johnstone
When exposed to the high energy X-ray and ultraviolet radiation of a very active star, water vapor in the upper atmospheres of planets can be photodissociated and rapidly lost to s…
Chromium isotope evidence in ejecta deposits for the nature of Paleoproterozoic impactors
Berengere Mougel, Frederic Moynier, Christa Gopel +1
Non-mass dependent chromium isotopic signatures have been successfully used to determine the presence and identification of extra-terrestrial materials in terrestrial impact rocks.…