Results 111 to 120 of about 59,386 (288)

The Caltech Core-Collapse Project (CCCP) [PDF]

, 2005
The cosmological utility of type Ia Supernovae prompted numerous studies of these events, and they are now well characterized observationally, both as individual objects and as a population. In contrast, all other types of supernovae (i.e.
Cenko, S. B., Fox, D. W., Gal-Yam, A., Leonard, D. C., Moon, D.-S., Sand, D. J., Soderberg, A. M.   +6 more
core  

Core-collapse supernovae

This is a pre-print of a chapter for the Encyclopedia of Astrophysics (edited by I. Mandel, section editor F.R.N.
Jerkstrand, Anders, Milisavljevic, Dan, Müller, Bernhard   +2 more
openaire   +2 more sources

High-cadence, early-time observations of core-collapse supernovae from the TESS prime mission [PDF]

, 2020
We present observations from the Transiting Exoplanet Survey Satellite (TESS) of twenty bright core-collapse supernovae with peak TESS-band magnitudes $\lesssim18$ mag.
P. Vallely, C. Kochanek, K. Stanek, M. Fausnaugh, B. Shappee   +4 more
semanticscholar   +1 more source

Explosive nucleosynthesis in core-collapse supernovae

, 2010
The specific mechanism and astrophysical site for the production of half of the elements heavier than iron via rapid neutron capture (r-process) remains to be found.
Almudena Arcones, Aoki W, Arcones A, Arcones A, Arcones A, Farouqi K, Freiburghaus C, Fröhlich C, Goriely S, Hoffman R D, Ishimaru Y, Ishimaru Y, Montes F, NuDat2, Otsuki K, Otsuki K, Pruet J, Qian Y Z, Qian Y Z, Qian Y Z, Thompson T A, Travaglio C, Wanajo S, Wanajo S, Wanajo S, Wanajo S, Wasserburg G J, Wasserburg G J, Witti J   +28 more
core   +1 more source

Astrophysics with core-collapse supernova gravitational wave signals in the next generation of gravitational wave detectors [PDF]

, 2019
The next generation of gravitational wave detectors will improve the detection prospects for gravitational waves from core-collapse supernovae. The complex astrophysics involved in core-collapse supernovae pose a significant challenge to modeling such ...
Frey, Ray, Heng, Ik Siong, Powell, Jade, Roma, Vincent   +3 more
core   +2 more sources

Managing and mitigating future public health risks: Planetary boundaries, global catastrophic risk, and inclusive wealth

Risk Analysis, Volume 45, Issue 7, Page 1607-1631, July 2025.
Abstract There are two separate conceptualizations for assessing existential risks: Planetary Boundaries (PBs) and global catastrophic risks (GCRs). While these concepts are similar in principle, their underpinning literatures tend not to engage with each other.
Eoin McLaughlin, Matthias Beck
wiley   +1 more source

A Slowly Pulsating Run‐Away B Star at High Galactic Latitude Ejected From a Spiral Arm

Astronomische Nachrichten, Volume 346, Issue 5, June 2025.
ABSTRACT We report the discovery of the young B6 V run‐away star LAMOST J083323.18 + 430825.4, 2.5 kpc above the Galactic plane. Its atmospheric parameters and chemical composition are determined from LAMOST spectra, indicating normal composition. Effective temperature (Teff$$ {T}_{\mathrm{eff}} $$ = 14,500$$ \mathrm{14,500} $$ K) and gravity (logg ...
Ulrich Heber, Maximilian Halenke, Aakash Bhat, Veronika Schaffenroth   +3 more
wiley   +1 more source

Hydrodynamic Mixing of Accretion Disk Outflows in Collapsars: Implications for r-process Signatures

The Astrophysical Journal, 2023
The astrophysical environments capable of triggering heavy-element synthesis via rapid neutron capture (the r -process) remain uncertain. While binary neutron star mergers (NSMs) are known to forge r -process elements, certain rare supernovae (SNe) have ...
Jennifer Barnes, Paul C. Duffell
doaj   +1 more source

Can We Draw Conclusions on Supernova Shock Wave Propagation Using Short‐Lived Radioactive Isotopes?

Astronomische Nachrichten, Volume 346, Issue 3-4, March-May 2025.
ABSTRACT We run a three‐dimensional Galactic chemical evolution (GCE) model to follow the propagation of 53Mn (exclusively produced from type Ia supernovae, SNIa), 60Fe (exclusively produced from core‐collapse supernovae, CCSNe), 182Hf (exclusively produced from intermediate mass stars, IMSs), and 244Pu (exclusively produced from neutron star mergers ...
Benjamin Wehmeyer, Andrés Yagüe López, Benoit Côté, Maria K. Petö, Chiaki Kobayashi, Maria Lugaro   +5 more
wiley   +1 more source

Including Neutrino-driven Convection in the Force Explosion Condition to Predict Explodability of Multidimensional Core-collapse Supernovae (FEC+)

The Astrophysical Journal
Most massive stars end their lives with core collapse. However, it is not clear which explode as a core-collapse supernova (CCSN), leaving behind a neutron star, and which collapse to a black hole, aborting the explosion.
Mariam Gogilashvili, Jeremiah W. Murphy, Jonah M. Miller   +2 more
doaj   +1 more source