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Third family of compact stars within a nonlocal chiral quark model equation of state
(American Physical Society, 2019-03)
A class of hybrid compact star equations of state is investigated that joins by a Maxwell construction a low-density phase of hadronic matter, modeled by a relativistic mean-field approach with excluded nucleon volume, ...
Constraints on the Physical Properties of GW190814 through Simulations Based on DECam Follow-up Observations by the Dark Energy Survey
(IOP Publishing Ltd, 2020-09)
On 2019 August 14, the LIGO and Virgo Collaborations detected gravitational waves from a black hole and a 2.6 solar mass compact object, possibly the first neutron star-black hole merger. In search of an optical counterpart, ...
Black hole fuelling in galaxy mergers: a high-resolution analysis
(Oxford, 2021)
Using parsec scale resolution hydrodynamical adaptive mesh refinement simulations, we have studied the mass transport process throughout a Galactic merger. The aim of such study is to connect both the peaks of mass accretion ...
Tail wavelets in merger of binary compact objects*
(Iop Publishing Ltd, 2020-07-01)
We present a model for tail wavelets, a phenomenon known as echo in the literature. The tail wavelet may appear in signal reconnaissances in the merger of binary compact objects, including black holes and neutron stars. ...
A parametric study on the formation of extended star clusters and ultra-compact dwarf galaxies
(2011)
Context. In the last decade, very extended old stellar clusters with masses in the range from a few 104 to 108 M⊙ have been found in various types of galaxies in different environments. Objects with masses comparable to ...
Delta baryons and diquark formation in the cores of neutron stars
(American Physical Society, 2020-09-09)
We investigate the hadron-quark phase transition in cold neutron stars in light of (i) the observed limits on the maximum-mass of heavy pulsars, (ii) constraints on the tidal properties inferred from the gravitational waves ...
GALAXY EVOLUTION IN A COMPLEX ENVIRONMENT: A MULTI-WAVELENGTH STUDY OF HCG 7
(IOP PUBLISHING LTD, 2010)
The environment where galaxies are found heavily influences their evolution. Close groupings, like the ones in the cores of galaxy clusters or compact groups, evolve in ways far more dramatic than their isolated counterparts. ...