The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am∗
The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am
- IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
- IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
The late time optical evolution of twelve core-collapse supernovae: detection of normal stellar winds
M Rizzo Smith, CS Kochanek… - Monthly Notices of the …, 2023 - academic.oup.com
We analyse the late time evolution of 12 supernovae (SNe) occurring over the last∼ 41 yr,
including nine Type IIP/L, two IIb, and one Ib/c, using UBVR optical data from the Large …
including nine Type IIP/L, two IIb, and one Ib/c, using UBVR optical data from the Large …
X-ray-luminous supernovae: threats to terrestrial biospheres
IR Brunton, C O'Mahoney, BD Fields… - The Astrophysical …, 2023 - iopscience.iop.org
The spectacular outbursts of energy associated with supernovae (SNe) have long motivated
research into their potentially hazardous effects on Earth and analogous environments …
research into their potentially hazardous effects on Earth and analogous environments …
On the lack of X-ray bright Type IIP supernovae
VV Dwarkadas - Monthly Notices of the Royal Astronomical …, 2014 - academic.oup.com
Type IIP supernovae (SNe) are expected to arise from red supergiant stars (RSGs). These
stars have observed mass-loss rates that span more than two orders of magnitude, from less …
stars have observed mass-loss rates that span more than two orders of magnitude, from less …
SRGA J181414. 6-225604: A New Galactic Symbiotic X-Ray Binary Outburst Triggered by an Intense Mass-loss Episode of a Heavily Obscured Mira Variable
We present the discovery and multiwavelength characterization of SRGA J181414. 6-
225604, a Galactic hard X-ray transient discovered during the ongoing SRG/ART-XC sky …
225604, a Galactic hard X-ray transient discovered during the ongoing SRG/ART-XC sky …
Probing final stages of stellar evolution with X-ray observations of SN 2013ej
Massive stars shape their surroundings with mass loss from winds during their lifetimes. Fast
ejecta from supernovae (SNe), from these massive stars, shock this circumstellar medium …
ejecta from supernovae (SNe), from these massive stars, shock this circumstellar medium …
Prospects for Time-Domain and Multi-Messenger Science with AXIS
The Advanced X-ray Imaging Satellite (AXIS) promises revolutionary science in the X-ray
and multi-messenger time domain. AXIS will leverage excellent spatial resolution (< 1.5 …
and multi-messenger time domain. AXIS will leverage excellent spatial resolution (< 1.5 …
The Chandra local volume survey. I. The X-ray point source populations of NGC 55, NGC 2403, and NGC 4214
B Binder, BF Williams, M Eracleous… - The Astronomical …, 2015 - iopscience.iop.org
We present comprehensive X-ray point source catalogs of NGC 55, NGC 2403, and NGC
4214 as part of the Chandra Local Volume Survey. The combined archival observations …
4214 as part of the Chandra Local Volume Survey. The combined archival observations …
A serendipitous discovery of GeV gamma-ray emission from supernova 2004dj in a survey of nearby star-forming galaxies with Fermi-LAT
SQ **, RY Liu, XY Wang, RZ Yang… - The Astrophysical …, 2020 - iopscience.iop.org
The interaction between a supernova ejecta and the circumstellar medium drives a strong
shock wave that accelerates particles (ie, electrons and protons). The radio and X-ray …
shock wave that accelerates particles (ie, electrons and protons). The radio and X-ray …
Radio Spectra of SN 2020oi: Effects of Radiative Cooling on the Deduced Source Properties
CI Björnsson - The Astrophysical Journal, 2022 - iopscience.iop.org
Observations of radiative cooling in a synchrotron source offer a possibility to further
constrain its properties. Inverse Compton cooling is indicated in the radio spectra during the …
constrain its properties. Inverse Compton cooling is indicated in the radio spectra during the …