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P. Lorén-Aguilar

22 papers hereh-index 17936 citations45 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author5
  • middle author12
  • last author4

Across the 21 of 22 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR11
  • astro-ph.EP4
  • astro-ph.HE3
  • astro-ph.GA2
  • astro-ph1
  • gr-qc1
same name
  • P. Lorén-Aguilar — 16 papers, h 9

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20032019
most citedA white dwarf cooling age of 8 Gyr for NGC 6791 from physical separation processes

243 citations · 1.1k across the 22 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.SR2018★ 57 cited

Double-Degenerate Carbon-Oxygen and Oxygen-Neon White Dwarf Mergers: A New Mechanism for Faint and Rapid Type Ia Supernovae

Rahul Kashyap, Tazkera Haque, Pablo Lorén-Aguilar +2

Type Ia supernovae (SNe Ia) originate from the thermonuclear explosion of carbon-oxygen white dwarfs (CO WDs), giving rise to luminous optical transients. A relatively common varie…

astro-ph.HE2018★ 19 cited

Electromagnetic emission of white dwarf binary mergers

J. A. Rueda, R. Ruffini, Y. Wang +6

It has been recently proposed that the ejected matter from white dwarf (WD) binary mergers can produce transient, optical and infrared emission similar to the "kilonovae" of neutro…

astro-ph.SR2018★ 19 cited

The Spin Evolution of Fast-Rotating, Magnetized Super-Chandrasekhar White Dwarfs in the Aftermath of White Dwarf Mergers

L. Becerra, J. A. Rueda, P. Loren-Aguilar +1

The evolution of the remnant of the merger of two white dwarfs is still an open problem. Furthermore, few studies have addressed the case in which the remnant is a magnetic white d…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.