Results 131 to 140 of about 2,618 (181)
Type II supernovae (SNe II) are the most frequently observed outcome of core-collapse explosions and provide a valuable window into the physical mechanisms governing the deaths of massive stars. However, estimates of explosion properties based on optical
Qiliang Fang +2 more
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We present follow-up imaging and spectroscopy and pre-explosion imaging of SN 2025pht located in NGC 1637 at 12 Mpc. Our spectroscopy shows that SN 2025pht is a Type II supernova (SN) with broad lines of hydrogen and with minimal line-of-sight extinction
Charles D. Kilpatrick +9 more
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Type Ia supernovae 2014J and 2011fe at the nebular phase [PDF]
© 2015, Pleiades Publishing, Inc. We present our observations and the results of our analysis of the nebular spectra for two nearby type Ia supernovae (SN 2014J and SN 2011fe).
Sunyaev R. +7 more
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SPY - the ESO Supernovae type Ia Progenitor survey [PDF]
Supernovae (SNe) mark the violent termination of a star’s life in an explosion. They are classified according to their light curve as type I or II, with the type I SNe producing very similar light curves, while the SNe type II are more diverse ...
Christlieb, N. +15 more
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We present and analyze panchromatic (0.35–14 μ m) spectroscopy of the Type II supernova 2023ixf, including near- and mid-infrared spectra obtained 33.6 days after explosion during the plateau phase, with the James Webb Space Telescope (JWST). This is the
J. M. DerKacy +48 more
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NEOWISE-R Caught the Luminous SN 2023ixf in Messier 101
During routine survey imaging, the reactivated Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE-R) serendipitously caught the Type II supernova SN 2023ixf in Messier 101 on the rise, starting day 3.6 through day 10.9, and again on the ...
Schuyler D. Van Dyk +18 more
doaj +1 more source
Type Ia supernovae 2014J and 2011fe at the nebular phase [PDF]
© 2015, Pleiades Publishing, Inc. We present our observations and the results of our analysis of the nebular spectra for two nearby type Ia supernovae (SN 2014J and SN 2011fe).
Sunyaev R. +7 more
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Discovery of a Likely Type II Supernova at z = 3.6 with JWST
Transient astronomy of the early, high-redshift ( z > 3) Universe is an unexplored regime that offers the possibility of probing the first stars and the epoch of reionization.
D. A. Coulter +32 more
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Analysis of 14 Years of X-Ray Emission from SN 2011DH
Ejecta from core-collapse supernovae interact with the circumstellar medium shed by the progenitor star, producing X-ray emission. Previous studies analyzed the X-ray spectrum of the Type IIb supernova SN 2011dh up to ∼500 days after explosion. Long-term
Elisa J. Gao, Vikram V. Dwarkadas
doaj +1 more source
The rise-time of Type II supernovae [PDF]
We investigate the early-time light curves of a large sample of 223 Type II supernovae (SNe II) from the Sloan Digital Sky Survey and the Supernova Legacy Survey.
Jaeger, Thomas de +16 more
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