activity
20172020
most citedA giant exoplanet orbiting a very low-mass star challenges planet formation models

130 citations · 199 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2020

The Effects of Asymmetric Dark Matter on Stellar Evolution I: Spin-Dependent Scattering

Troy J. Raen, Héctor Martínez-Rodríguez, Travis J. Hurst +3

Most of the dark matter (DM) search over the last few decades has focused on WIMPs, but the viable parameter space is quickly shrinking. Asymmetric Dark Matter (ADM) is a WIMP-like…

astro-ph.HE20207 cited

Evidence of a Type Ia Progenitor for Supernova Remnant 3C 397

Héctor Martínez-Rodríguez, Laura A. Lopez, Katie Auchettl +6

The explosive origin of the young supernova remnant (SNR) 3C 397 (G41.1-0.3) is debated. Its elongated morphology and proximity to a molecular cloud are suggestive of a core-collap…

astro-ph.EP201944 cited

Exomoons in the habitable zones of M dwarfs

Héctor Martínez-Rodríguez, José Antonio Caballero, Carlos Cifuentes +2

M dwarfs host most of the exoplanets in the local Milky Way. Some of these planets, ranging from sub-Earths to super-Jupiters, orbit in their stars' habitable zones (HZs), although…

astro-ph.EP2019130 cited

A giant exoplanet orbiting a very low-mass star challenges planet formation models

J. C. Morales, A. J. Mustill, I. Ribas +179

Statistical analyses from exoplanet surveys around low-mass stars indicate that super-Earth and Neptune-mass planets are more frequent than gas giants around such stars, in agreeme…

astro-ph.SR2018

SNR-calibrated Type Ia supernova models

Eduardo Bravo, Carles Badenes, Héctor Martínez-Rodríguez

Current Type Ia supernova (SN Ia) models can reproduce most visible+IR+UV observations. In the X-ray band, the determination of elemental abundance ratios in supernova remnants (SN…

astro-ph.HE2018

Chandrasekhar and sub-Chandrasekhar models for the X-ray emission of Type Ia supernova remnants (I): Bulk properties

Héctor Martínez-Rodríguez, Carles Badenes, Shiu-Hang Lee +9

Type Ia supernovae originate from the explosion of carbon-oxygen white dwarfs in binary systems, but the exact nature of their progenitors remains elusive. The bulk properties of T…