activity
20152026
most citedPainting a portrait of the Galactic disc with its stellar clusters

554 citations · 1.4k across the 56 of their papers we have counts for

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Showing 2024Show all

10 papers · 1 filter

astro-ph.SR2024

Two young eclipsing binaries in Orion with temperatures and radii affected by spots and third bodies

Marina Kounkel, Keivan G. Stassun

In this work we present a model of two young eclipsing binaries in the Orion Complex. Both heavily spotted, they present radii and temperatures that are in disagreement with the pr…

astro-ph.SR2024

Atmospheric parameters and chemical abundances within 100 pc. A sample of G, K, and M main-sequence stars

Ricardo López-Valdivia, Lucía Adame, Eduardo Zagala Lagunas +9

To date, we have access to enormous inventories of stellar spectra that allow the extraction of atmospheric parameters and chemical abundances essential in stellar studies. However…

astro-ph.EP20241 cited

The TEMPO Survey II: Science Cases Leveraged from a Proposed 30-Day Time Domain Survey of the Orion Nebula with the Nancy Grace Roman Space Telescope

Melinda Soares-Furtado, Mary Anne Limbach, Andrew Vanderburg +26

The TEMPO (Transiting Exosatellites, Moons, and Planets in Orion) Survey is a proposed 30-day observational campaign using the Nancy Grace Roman Space Telescope. By providing deep,…

astro-ph.SR2024

The evolution of stellar X-ray activity and angular momentum as seen by eROSITA, TESS, and Gaia

Keivan G. Stassun, Marina Kounkel

We have assembled a sample of 8200 stars with spectral types F5V-M5V, all having directly measured X-ray luminosities from eROSITA and rotation periods from TESS, and having…

astro-ph.GA2024

SDSS-V Local Volume Mapper (LVM): A Glimpse into Orion

K. Kreckel, O. V. Egorov, E. Egorova +37

The Orion Molecular Cloud complex, one of the nearest (D = 406 pc) and most extensively studied massive star-forming regions, is ideal for constraining the physics of stellar feedb…

astro-ph.SR2024

Protostellar spin-up and fast rotator formation through binary star formation

Rajika L. Kuruwita, Christoph Federrath, Marina Kounkel

(Edited) Many fast rotator stars (rotation periods of < 2 days) are found in unresolved binaries with separations of tens of au. This correlation leads to the question of whether t…