Core-collapse supernovae from 9 to 120 solar masses based on neutrino-powered explosions
T Sukhbold, T Ertl, SE Woosley, JM Brown… - The Astrophysical …, 2016 - iopscience.iop.org
Nucleosynthesis, light curves, explosion energies, and remnant masses are calculated for a
grid of supernovae (SNe) resulting from massive stars with solar metallicity and masses from …
grid of supernovae (SNe) resulting from massive stars with solar metallicity and masses from …
The allowed parameter space of a long-lived neutron star as the merger remnant of GW170817
Due to the limited sensitivity of the current gravitational wave (GW) detectors, the central
remnant of the binary neutron star (NS) merger associated with GW170817 remains an open …
remnant of the binary neutron star (NS) merger associated with GW170817 remains an open …
Gaia17biu/SN 2017egm in NGC 3191: the closest hydrogen-poor superluminous supernova to date is in a “normal,” massive, metal-rich spiral galaxy
Hydrogen-poor superluminous supernovae (SLSNe-I) have been predominantly found in
low-metallicity, star-forming dwarf galaxies. Here we identify Gaia17biu/SN 2017egm as an …
low-metallicity, star-forming dwarf galaxies. Here we identify Gaia17biu/SN 2017egm as an …
Internal x-ray plateau in short GRBs: Signature of supramassive fast-rotating quark stars?
A supramassive, strongly magnetized millisecond neutron star (NS) has been proposed to
be the candidate central engine of at least some short gamma-ray bursts (SGRBs), based on …
be the candidate central engine of at least some short gamma-ray bursts (SGRBs), based on …
The Luminosity Function of Tidal Disruption Flares for the ZTF-I Survey
The high-cadence survey of the Zwicky Transient Facility (ZTF) has completely dominated
the discovery of tidal disruption events (TDEs) in the past few years and resulted in the …
the discovery of tidal disruption events (TDEs) in the past few years and resulted in the …
Explaining the most energetic supernovae with an inefficient jet-feedback mechanism
We suggest that the energetic radiation from core-collapse super-energetic supernovae
(SESNe) is due to a long-lasting accretion process onto the newly born neutron star (NS) …
(SESNe) is due to a long-lasting accretion process onto the newly born neutron star (NS) …
R-mode Stability of GW190814's Secondary Component as a Supermassive and Superfast Pulsar
The nature of GW190814's secondary component m 2 of mass 2.50–2.67 M⊙ in the mass
gap between the currently known maximum mass of neutron stars and the minimum mass of …
gap between the currently known maximum mass of neutron stars and the minimum mass of …
X-Rays from the Location of the Double-humped Transient ASASSN-15lh
R Margutti, BD Metzger, R Chornock… - The Astrophysical …, 2017 - iopscience.iop.org
We present the detection of persistent soft X-ray radiation with ${L} _ {x}\sim {10}^{41} $–10
42 erg s–1 at the location of the extremely luminous, double-humped transient ASASSN …
42 erg s–1 at the location of the extremely luminous, double-humped transient ASASSN …
Results from a systematic survey of X-ray emission from hydrogen-poor superluminous SNe
R Margutti, R Chornock, BD Metzger… - The Astrophysical …, 2018 - iopscience.iop.org
We present the results from a sensitive X-ray survey of 26 nearby hydrogen-poor
superluminous supernovae (SLSNe-I) with Swift, Chandra, and XMM. This data set …
superluminous supernovae (SLSNe-I) with Swift, Chandra, and XMM. This data set …
A statistical study of superluminous supernovae using the magnetar engine model and implications for their connection with gamma-ray bursts and hypernovae
By fitting the bolometric light curves of 31 superluminous supernovae (SLSNe) with the
magnetar engine model, we derive the ejecta masses and magnetar parameters for these …
magnetar engine model, we derive the ejecta masses and magnetar parameters for these …