activity
20072021
most citedAbundances of the elements in the solar system

534 citations · 1.3k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.EP2021★ 22 cited

Evolution of the parent body of enstatite (EL) chondrites

Mario Trieloff, Jens Hopp, Hans-Peter Gail

Chondrites stem from undifferentiated asteroidal parent bodies that nevertheless experienced a certain degree of metamorphism after their formation in the early solar system. Maxim…

astro-ph.SR2020★ 1 cited

Non-stoichiometric amorphous magnesium-iron silicates in circumstellar dust shells. Dust growth in outflows from supergiants

Hans-Peter Gail, Akemi Tamanai, Annemarie Pucci +1

We investigate the dust growth in oxygen-rich stellar outflows for a set of nine well-observed massive supergiants with optically thin dust shells. Models of the infrared emission…

astro-ph.SR2020★ 2 cited

Extended view on the dust shells around two carbon stars

M. Mečina, B. Aringer, W. Nowotny +4

Stars on the asymptotic giant branch (AGB) lose considerable amounts of matter through their dust-driven stellar winds. A number of such sources have been imaged by Herschel/PACS,…

astro-ph.EP2019★ 37 cited

Thermal history modeling of the L chondrite parent body

Hans-Peter Gail, Mario Trieloff

The radius of the L chondrite parent body, its formation time, and its evolution history are determined by fitting theoretical models to empirical data of radioisotopic chronometer…

astro-ph.EP2018★ 7 cited

Thermal evolution and sintering of chondritic planetesimals IV. Temperature dependence of heat conductivity of asteroids and meteorites

Hans-Peter Gail, Mario Trieloff

Understanding the compaction and differentiation of the planetesimals and protoplanets from the Asteroid Belt and the terrestrial planet region of the Solar System requires a relia…

astro-ph.EP2017★ 65 cited

The spatial distribution of carbon dust in the early solar nebula and the carbon content of planetesimals

Hans-Peter Gail, Mario Trieloff

A high fraction of carbon bound in solid carbonaceous material is observed to exist in bodies formed in the cold outskirts of the solar nebula, while bodies in the terrestrial plan…