activity
19972025
most citedConvectively driven vortex flows in the Sun

214 citations · 810 across the 31 of their papers we have counts for

collaborators

31 papers

astro-ph.GA2025★ 2 cited

Constraints on dark matter models from the stellar cores observed in ultra-faint dwarf galaxies: Self-interacting dark matter

Jorge Sanchez Almeida

It has been proposed that the stellar cores observed in ultra-faint dwarf (UFD) galaxies reflect underlying dark matter (DM) cores that cannot be formed by stellar feedback acting…

astro-ph.GA2025★ 1 cited

Constraining the shape of dark matter haloes using only starlight. I. A new technique and its application to the galaxy Nube

Jorge Sanchez Almeida, Ignacio Trujillo, Mireia Montes +1

We present a new technique to constrain the gravitational potential of a galaxy from the observed stellar mass surface density alone under a number of assumptions. It uses the clas…

astro-ph.HE2024★ 33 cited

Dynamical confirmation of a black hole in the X-ray transient Swift J1727.8-1613

D. Mata Sanchez, M. A. P. Torres, J. Casares +3

The X-ray transient Swift J1727.8-1613 ended its 10-month discovery outburst on June of 2024, when it reached an optical brightness comparable to pre-discovery magnitudes. With the…

astro-ph.EP2024★ 8 cited

Validation of a Third Planet in the LHS 1678 System

Michele L. Silverstein, Thomas Barclay, Joshua E. Schlieder +24

The nearby LHS 1678 (TOI-696) system contains two confirmed planets and a wide-orbit, likely-brown-dwarf companion, which orbit an M2 dwarf with a unique evolutionary history. The…

astro-ph.EP2023★ 2 cited

Glancing through the debris disk: Photometric analysis of DE Boo with CHEOPS

Á. Boldog, Gy. M. Szabó, L. Kriskovics +76

DE Boo is a unique system, with an edge-on view through the debris disk around the star. The disk, which is analogous to the Kuiper belt in the Solar System, was reported to extend…

astro-ph.GA2022★ 5 cited

Dwarf galaxies with central cores in modified Newtonian dynamics (MOND) gravity

J. Sanchez Almeida

Some dwarf galaxies are within the Mondian regime at all radii, i.e., the gravitational acceleration provided by the observed baryons is always below the threshold of $g_†\simeq 1.…