196 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Adolfo Ibáñez UniversityCL32 papers
- Millennium Institute of AstrophysicsCL29 papers
- European Southern ObservatoryCL17 papers
- Pontificia Universidad Católica de ChileCL17 papers
- Max Planck Institute for AstronomyDE15 papers
- University of ChileCL15 papers
- Center for Astrophysics Harvard & SmithsonianUS13 papers
- Massachusetts Institute of TechnologyUS13 papers
- Princeton UniversityUS12 papers
- Ames Research CenterUS11 papers
- American Institute of Aeronautics and AstronauticsUS10 papers
- California Institute of TechnologyUS9 papers
5 papers · 1 filter
Polycyclic aromatic hydrocarbon (PAH) abundances in the disk around T Chamaeleontis (T Cha): PAH sizes, ionization fraction, and mass during JWST observations
Rahul Bandyopadhyay, Simon Casassus
The T Tauri star T Cha is known to have a protoplanetary disk with a dust gap separating the inner and outer disk regions. The mid-infrared JWST spectrum of T Cha shows multiple pr…
NGTS-EB-7, an eccentric, long-period, low-mass eclipsing binary
Toby Rodel, Christopher. A. Watson, Solène Ulmer-Moll +35
Despite being the most common types of stars in the Galaxy, the physical properties of late M dwarfs are often poorly constrained. A trend of radius inflation compared to evolution…
Spectroscopic observations of flares and superflares on AU Mic
P. Odert, M. Leitzinger, R. Greimel +13
The young active flare star AU~Mic is the planet host star with the highest flare rate from TESS data. Therefore, it represents an ideal target for dedicated ground-based monitorin…
The EBLM Project XII. An eccentric, long-period eclipsing binary with a companion near the hydrogen-burning limit
Yasmin T. Davis, Amaury H. M. J. Triaud, Alix V. Freckelton +17
In the hunt for Earth-like exoplanets it is crucial to have reliable host star parameters, as they have a direct impact on the accuracy and precision of the inferred parameters for…
Resolving the Binary Components of the Outbursting Protostar HBC 494 with ALMA
Pedro Henrique Nogueira, Alice Zurlo, Sebastián Pérez +15
Episodic accretion is a low-mass pre-main sequence phenomenon characterized by sudden outbursts of enhanced accretion. These objects are classified into two: protostars with elevat…