Browsing by Author "Lorén Aguilar, Pablo"
Now showing items 1-18 of 18
-
3D Hydrodynamical simulations of helium-ignited double-degenerate white dwarf mergers
Roy, Niranjan C.; Tiwari, Vishal; Bobrick, Alexey; Kosakowski, Daniel; Fisher, Robert; Perets, Hagai B.; Kashyap, Rahul; Lorén Aguilar, Pablo; García-Berro Montilla, Enrique (2022-06-01)
Article
Open AccessThe origins of Type Ia supernovae (SNe Ia) are still debated. Some of the leading scenarios involve a double detonation in double white dwarf (WD) systems. In these scenarios, helium shell detonation occurs on top of a ... -
A common origin of magnetism from planets to white dwarfs
Isern Vilaboy, Jordi; García-Berro Montilla, Enrique; Kulebi, Baybar; Lorén Aguilar, Pablo (2017-02-20)
Article
Open AccessIsolated magnetic white dwarfs have field strengths ranging from kilogauss to gigagauss. However, the origin of the magnetic field has not been hitherto elucidated. Whether these fields are fossil, hence the remnants of ... -
A white dwarf merger as progenitor of the anomalous X-Ray pulsar 4U 0142+61?
Rueda, Jorge A.; Boshkayev, K.; Izzo, L.; Ruffini, R.; Lorén Aguilar, Pablo; Kuelebi, B.; Aznar Siguan, Gabriela; García-Berro Montilla, Enrique (2013-08)
Article
Open AccessIt has been recently proposed that massive, fast-rotating, highly magnetized white dwarfs could describe the observational properties of some of soft gamma-ray repeaters and anomalous X-ray pulsars (AXPs). Moreover, it has ... -
BAETULO XXI, o de com arribar a Mart des de la secundària
Serrano Porta, Lydia; Ramírez Alcántara, Jorge; Portell Canal, Xavier; Pijuan, Caterina; Monfort Peligero, Lluís; Ayza, Assumpta; Berenguer Sau, Jordi; Carnerero López, Sheila; Crespo Artiaga, Daniel; López Codina, Daniel; López Rubio, Juan; Lorén Aguilar, Pablo; Melo Vera, Maria Jesús (2008)
Conference report
Open Access -
Detonations in white dwarf dynamical interactions
Aznar Siguan, Gabriela; García-Berro Montilla, Enrique; Lorén Aguilar, Pablo; José Pont, Jordi; Isern Vilaboy, Jordi (2013)
Article
Open Accessn old, dense stellar systems collisions of white dwarfs are a rather frequent phenomenon. Here we present the results of a comprehensive set of Smoothed Particle Hydrodynamics simulations of close encounters of white ... -
Double degenerate mergers as progenitors of high-field magnetic white dwarfs
García-Berro Montilla, Enrique; Lorén Aguilar, Pablo; Aznar Siguan, Gabriela; Torres Gil, Santiago; Camacho Díaz, Judit; Althaus, Leandro Gabriel; Córsico, Alejando Hugo; Kulebi, Baybar; Isern Vilaboy, Jordi (2011-04-10)
Article
Open AccessHigh-field magnetic white dwarfs have been long suspected to be the result of stellar mergers. However, the nature of the coalescing stars and the precise mech anism that produces the magnetic field are still unknown. ... -
Electromagnetic emission of white dwarf binary mergers
Rueda Hernández, Jorge Armando; Ruffini, R.; Wang, Yu; Bianco, C. L.; Blanco Iglesias, José Miguel; Karlica, Mile; Lorén Aguilar, Pablo; Moradi, R.; Sahakyan, N. (2019-03-29)
Article
Open AccessIt 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 neutron star (NS) binary mergers. To confirm ... -
High-resolution smoothed particle hydrodynamics simulations of the merger of binary white dwarfs
Lorén Aguilar, Pablo; Isern Vilaboy, Jordi; García-Berro Montilla, Enrique (2009-06)
Article
Open AccessContext. The coalescence of two white dwarfs is the final outcome of a sizeable fraction of binary stellar systems. Moreover, this process has been proposed to explain several interesting astrophysical phenomena. Aims. ... -
Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars
Longland, Richard Leigh; Lorén Aguilar, Pablo; José Pont, Jordi; García-Berro Montilla, Enrique; Althaus, Leandro Gabriel; Isern Vilaboy, Jordi (2011-08-20)
Article
Restricted access - publisher's policyMany hydrogen-deficient stars are characterized by surface abundance patterns that are hard to reconcile with conventional stellar evolution. Instead, it has been suggested that they may represent the result of a merger ... -
On the origin of high-field magnetic white dwarfs
García-Berro Montilla, Enrique; Torres Gil, Santiago; Lorén Aguilar, Pablo; Aznar Siguan, Gabriela; Camacho Díaz, Judit; Kulebi, Baybar; Isern Vilaboy, Jordi; Althaus, Leandro Gabriel; Corsico, Alejandro H. (Astronomical Society of the Pacific, 2013-01-01)
Conference lecture
Open AccessEvery two years, white dwarf researchers and enthusiasts meet to exchange their knowledge and discuss recent developments in white dwarf theory and observations. These proceedings are from the 18th European White Dwarf ... -
One-armed spiral instability in double-degenerate post-merger accretion disks
kashyap, Rahul; Fisher, Robert T.; García-Berro Montilla, Enrique; Aznar-Siguán, Gabriela; Ji, Suoqing; Lorén Aguilar, Pablo (2017-05-01)
Article
Open AccessIncreasing observational and theoretical evidence points to binary white dwarf (WD) mergers as the origin of some, if not most, normal Type Ia supernovae (SNe Ia). In this paper, we discuss the post-merger evolution of ... -
Self-gravitating barotropic equilibrium configurations of rotating bodies with smoothed particle hydrodynamics
García Senz, Domingo; Cabezón Gómez, Rubén Martín; Blanco Iglesias, José Miguel; Lorén Aguilar, Pablo (EDP Sciences, 2020-05-14)
Article
Open Access -
Smoothed particle hydrodynamics simulations of the core-degenerate scenario for Type Ia supernovae
Aznar Siguan, Gabriela; García-Berro Montilla, Enrique; Lorén Aguilar, Pablo; Soker, Noam; Kashi, Amit (2015-07-01)
Article
Open AccessThe core-degenerate scenario for Type Ia supernovae involves the merger of the hot core of an asymptotic giant branch star and a white dwarf, and might contribute a non-negligible fraction of all thermonuclear supernovae. ... -
Spiral instability can drive thermonuclear explosions in binary white dwarf mergers
kashyap, Rahul; Fisher, Robert T.; García-Berro Montilla, Enrique; Aznar Siguan, Gabriela; Ji, Suoqing; Lorén Aguilar, Pablo (2015-02-10)
Article
Open AccessThermonuclear, or Type Ia supernovae (SNe Ia), originate from the explosion of carbon-oxygen white dwarfs, and serve as standardizable cosmological candles. However, despite their importance, the nature of the progenitor ... -
The gravitational wave emission from white dwarf interactions in globular clusters
Lorén Aguilar, Pablo; Lobo Gutiérrez, José Alberto; Isern Vilaboy, Jordi; García-Berro Montilla, Enrique (2009-03-01)
Article
Restricted access - publisher's policyIn the dense central regions of globular clusters close encounters of two white dwarfs are relatively frequent. The estimated frequency is one or more strong encounters per star in the lifetime of the cluster. Such ... -
The post-merger magnetized evolution of white dwarf binaries: The double-degenerate channel of sub-Chandrasekhar type Ia supernovae and the formation of magnetized white dwarfs
Ji, Suoqing; Fisher, Robert T.; García-Berro Montilla, Enrique; Tzeferacos, Petros; Jordan, George C.; Lee, Dongwook; Lorén Aguilar, Pablo; Cremer, Pascal; Behrends, Jan (2013-08-20)
Article
Open AccessType Ia supernovae (SNe Ia) play a crucial role as standardizable cosmological candles, though the nature of their progenitors is a subject of active investigation. Recent observational and theoretical work has pointed to ... -
White dwarf dynamical interactions and fast optical transients
García-Berro Montilla, Enrique; Badenes Montoliu, Carles; Aznar Siguan, Gabriela; Lorén Aguilar, Pablo (2017-07-01)
Article
Open AccessRecent advances in time-domain astronomy have uncovered a new class of optical transients with time-scales shorter than typical supernovae and a wide range of peak luminosities. Several subtypes have been identified within ... -
White dwarf mergers and the origin of R coronae borealis stars
Lorén Aguilar, Pablo; Longland, Richard Leigh; José Pont, Jordi; García-Berro Montilla, Enrique; Althaus, Leandro Gabriel; Isern-Fontanet, J. (2012)
Conference report
Restricted access - publisher's policyWe present a nucleosynthesis study of the merger of a 0.4 M⊙ helium white dwarf with a 0.8 M⊙ carbon-oxygen white dwarf, coupling the thermodynamic history of Smoothed Particle Hydrodynamics particles with a post-processing ...