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- University of MichiganUS83 papers
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- Centre National de la Recherche ScientifiqueFR22 papers
- National ObservatoryBR22 papers
- Instituto de Astrofísica de AndalucíaES19 papers
- Valongo ObservatoryBR18 papers
- Universidade Federal do Rio de JaneiroBR17 papers
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- Centro de Estudios de Física del Cosmos de AragónES13 papers
- Donostia International Physics CenterES13 papers
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- Aix-Marseille UniversitéFR12 papers
8 papers · 1 filter
Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
D. Pauli, L. M. Oskinova, W. -R. Hamann +16
The origin of the observed population of Wolf-Rayet (WR) stars in low-metallicity (low-Z) galaxies, such as the Small Magellanic Cloud (SMC), is not yet understood. Standard, singl…
The Evolution Of The Inner Regions of Protoplanetary Disks
Ezequiel Manzo-Martínez, Nuria Calvet, Jesús Hernández +6
We present a study of the evolution of the inner few astronomical units of protoplanetary disks around low-mass stars. We consider nearby stellar groups with ages spanning from 1 t…
Irregular dust features around intermediate-mass young stars with GPI: signs of youth or misaligned disks?
Anna S. E. Laws, Tim J. Harries, Benjamin R. Setterholm +14
We are undertaking a large survey of over thirty disks using the Gemini Planet Imager (GPI) to see whether the observed dust structures match spectral energy distribution (SED) pre…
A high resolution mid-infrared survey of water emission from protoplanetary disks
Colette Salyk, John Lacy, Matt Richter +5
We present the largest survey of spectrally resolved mid-infrared water emission to date, with spectra for 11 disks obtained with the Michelle and TEXES spectrographs on Gemini Nor…
Dust-trapping vortices and a potentially planet-triggered spiral wake in the pre-transitional disk of V1247 Orionis
Stefan Kraus, Alexander Kreplin, Misato Fukagawa +8
The radial drift problem constitutes one of the most fundamental problems in planet formation theory, as it predicts particles to drift into the star before they are able to grow t…
A high-mass protobinary system with spatially resolved circumstellar accretion disks and circumbinary disk
Stefan Kraus, Jacques Kluska, Alexander Kreplin +9
High-mass multiples might form via fragmentation of self-gravitational disks or alternative scenarios such as disk-assisted capture. However, only few observational constraints exi…