Results 111 to 120 of about 7,219,823 (215)

Atomic gas properties at the positions of Type Ia, II, and Ib/c supernovae

Astronomy & Astrophysics
Context. Understanding which stars explode as which type of supernova (SN) is crucial to measure their contribution to the metal production and feedback halting star formation.
Šlaus Bruno, Gotkiewicz Natalia, Michałowski Michał J., Leśniewska Aleksandra, Nowaczyk Przemysław, Ryzhov Oleh, Solar Martín, Nadolny Jakub, Dimitrov Wojciech   +8 more
doaj   +1 more source

Late Jets, Early Sparks: Illuminating the Premaximum Bumps in Superluminous Supernovae

The Astrophysical Journal Letters
Superluminous supernovae (SLSNe) radiate ≳10–100 times more energy than ordinary stellar explosions, implicating a novel power source behind these enigmatic events.
Ore Gottlieb, Brian D. Metzger
doaj   +1 more source

Bridging the gap between SLSNe and SE-SNe

Astronomy & Astrophysics
The Type I super-luminous supernova SN 2024jlc (ZTF24aapadbb) exploded on 25 May 2024 at z = 0.039. This was the closest supernova of this class discovered in recent years and one of the closest ever.
Simongini A., Acero F., Imbrogno M., Wise J. L., Sollerman J., Schulze S., Kuin N. P. M., Chen T. X., Fremling C., Gangopadhyay A., Kasliwal M. M., Laher R. R., McGrath Z., Perley D. A., Purdum J. N., Rehemtulla N., Rich R. M., Riddle R.   +17 more
doaj   +1 more source

Evolutionary Models for Type Ib/c Supernova Progenitors [PDF]

Publications of the Astronomical Society of Australia, 2015
AbstractSNe Ib/c mark the deaths of hydrogen-deficient massive stars. The evolutionary scenarios for SNe Ib/c progenitors involve many important physical processes including mass loss by winds and its metallicity dependence, stellar rotation, and binary interactions. This makes SNe Ib/c an excellent test bed for stellar evolution theory.
openaire   +2 more sources

Constraints on Type Ib/c Supernovae and Gamma-Ray Burst Progenitors

, 2015
Although there is strong support for the collapsar engine as the power source of long-duration gamma-ray bursts (GRBs), we still do not definitively know the progenitor of these explosions.
Nomoto, Ken'ichi, Mazzali, Paolo A, Prochaska, Jason, Rockefeller, Gabe, Chevalier, Roger A, Schmidt, Brian, van Putten, Maurice, Fryer, Chris L, Berger, Edo, van den Heuvel, Ed P. J., Cappellaro, Enrico, Kulkarni, Shrinivas R, Young, Patrick, Panaitescu, Alin, Hungerford, Aimee, Yoon, Sung-Chui, Podsiadlowski, Ph.   +16 more
core   +1 more source

Multifilter UV to Near-infrared Data-driven Light-curve Templates for Stripped-envelope Supernovae

The Astrophysical Journal Supplement Series
While the spectroscopic classification scheme for stripped-envelope supernovae (SESNe) is clear, and we know that they originate from massive stars that lost some or all of their envelopes of hydrogen and helium, the photometric evolution of classes ...
Somayeh Khakpash, Federica B. Bianco, Maryam Modjaz, Willow F. Fortino, Alexander Gagliano, Conor Larison, Tyler A. Pritchard   +6 more
doaj   +1 more source

Fast radio bursts as standard candles for cosmology

Physics Letters B
Recently, fast radio bursts (FRBs) have become a thriving field in astronomy and cosmology. Due to their extragalactic and cosmological origin, they are useful to study the cosmic expansion and the intergalactic medium (IGM).
Han-Yue Guo, Hao Wei
doaj   +1 more source

Type Ibn supernovae from ultra-stripped supernova progenitors

<jats:title>Abstract</jats:title> <jats:p>Ultra-stripped supernovae are core-collapse supernovae from progenitors that lose a significant fraction of mass because of the binary interactions with their compact companion stars.
Müller, Bernhard, Sorokina, Elena I, Ushakova, Marina, Heger, Alexander, Moriya, Takashi J, Blinnikov, Sergei I, Tauris, Thomas M; id_orcid   +6 more
core   +1 more source

86th Annual Meeting of the Meteoritical Society (2024)

Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley   +1 more source

SN 2023zaw: An Ultrastripped, Nickel-poor Supernova from a Low-mass Progenitor

The Astrophysical Journal Letters
We present SN 2023zaw—a subluminous ( M _r = −16.7 mag) and rapidly evolving supernova ( t _1/2, _r = 4.9 days), with the lowest nickel mass (≈0.002 M _⊙ ) measured among all stripped-envelope supernovae discovered to date.
Kaustav K. Das, Christoffer Fremling, Mansi M. Kasliwal, Steve Schulze, Jesper Sollerman, Viraj Karambelkar, Sam Rose, Shreya Anand, Igor Andreoni, Marie Aubert, Sean J. Brennan, S. Bradley Cenko, Michael W. Coughlin, B. O’Connor, Kishalay De, Jim Fuller, Matthew Graham, Erica Hammerstein, Annastasia Haynie, K-Ryan Hinds, Io Kleiser, S. R. Kulkarni, Zeren Lin, Chang Liu, Ashish A. Mahabal, Christopher Martin, Adam A. Miller, James D. Neill, Daniel A. Perley, Priscila J. Pessi, Nikolaus Z. Prusinski, Josiah Purdum, Vikram Ravi, Ben Rusholme, Samantha Wu, Avery Wold, Lin Yan   +36 more
doaj   +1 more source