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Several supernova remnants and young neutron stars were recently discovered relatively high above the Galactic plane. One possibility is that they originate from runaway OB stars born in the Galactic disk. Understanding their origin will…

太阳与恒星天体物理 · 物理学 2025-08-28 Vinka Dakić , Sergei B. Popov , Roberto Turolla

Cosmic explosions dissipate energy into their surroundings on a very wide range of time-scales: producing shock waves and associated particle acceleration. The historical culprits for the acceleration of the bulk of Galactic cosmic rays are…

高能天体物理现象 · 物理学 2015-06-12 J. A. Hinton , R. L. C. Starling

Cosmic radiation backgrounds are a constraint on life, and their distribution will affect the Galactic Habitable Zone. Life on Earth has developed in the context of these backgrounds, and characterizing event rates will elaborate the…

地球与行星天体物理 · 物理学 2011-05-23 Adrian L. Melott , Brian C. Thomas

The passage of the Earth through dense clumps of dark matter, the presence of which are predicted by certain cosmologies, would produce large quantities of heat in the interior of this planet through the capture and subsequent annihilation…

天体物理学 · 物理学 2011-05-23 Samar Abbas , Afsar Abbas

We have reevaluated recent studies of the effects on Earth by cosmic rays (CRs) from nearby supernovae (SNe) at 100 and 50 pc, in the diffusive transport CR case, here including an early-time suppression at lower CR energies neglected in…

地球与行星天体物理 · 物理学 2023-06-16 Brian C. Thomas , Alexander M. Yelland

Supernovae release an enormous amount of energy into the interstellar medium. Their remnants can observationally be traced up to several ten-thousand years. So far more than 230 Galactic supernova remnants (SNRs) have been identified in the…

天体物理学 · 物理学 2007-05-23 W. Reich

Supernovae and their remnants are believed to be prodigious sources of Galactic cosmic rays and interstellar dust. Understanding the mechanisms behind their surprisingly high production rate is helped by the study of nearby young supernova…

高能天体物理现象 · 物理学 2015-06-17 L. Staveley-Smith , T. M. Potter , G. Zanardo , B. M. Gaensler , C. -Y. Ng

Extragalactic transient searches have historically been limited to looking for the appearance of new sources such as supernovae. It is now possible to carry out a new kind of survey that will do the opposite, that is, search for the…

天体物理学 · 物理学 2010-11-11 C. S. Kochanek , J. F. Beacom , M. D. Kistler , J. L. Prieto , K. Z. Stanek , T. A. Thompson , H. Yuksel

The observed value $\Lambda_{\rm obs}$ of the cosmological constant $\Lambda$ is extremely smaller than theoretical expectations, and the anthropic argument has been proposed as a solution to this problem because galaxies do not form when…

宇宙学与河外天体物理 · 物理学 2019-10-09 Tomonori Totani , Hidetoshi Omiya , Takahiro Sudoh , Masakazu A. R. Kobayashi , Masahiro Nagashima

The detection of $\sim 1.5-3.2$ Myr old $^{60}$Fe on Earth indicates recent nearby core-collapse supernovae. For supernovae in multiple stars, the primary stars may become neutron stars, while former companions may become unbound and become…

高能天体物理现象 · 物理学 2019-10-02 Ralph Neuhaeuser , Frank Gießler , Valeri V. Hambaryan

Our arguments deal with the early evolution of Galactic globular clusters and show why only a few of the supernovae products were retained within globular clusters and only in the most massive cases ($M \ge 10^6$ Msol), while less massive…

星系天体物理 · 物理学 2015-11-11 Guillermo Tenorio-Tagle , Casiana Munoz-Tunon , Sergiy Silich , Santi Cassisi

The activity of massive stars approaching core-collapse can strongly affect the appearance of the star and its subsequent supernova. Late-phase convective nuclear burning generates waves that propagate toward the stellar surface, heating…

高能天体物理现象 · 物理学 2023-05-10 Shing-Chi Leung , Jim Fuller

Recent observations suggest that many planetary-mass objects may be present in the outer solar system between the Kuiper belt and the Oort cloud. Gravitational perturbations may occasionally bring them into the inner solar system. Their…

天体物理学 · 物理学 2007-05-23 Daniele Fargion , Arnon Dar

Live $^{60}$Fe has recently been reported in a deep-ocean ferromanganese crust. Analysis of the isotopic ratios in the sample suggests that the measured $^{60}$Fe abundance exceeds the levels generated by terrestrial and cosmogenic sources,…

天体物理学 · 物理学 2009-09-11 Brian D. Fields , John Ellis

We have made VLA images of the fields around three young pulsars which have resulted in the discovery of two new supernova remnants and confirmation of a third. We argue that, in at least two cases and perhaps the third, the pulsars are…

天体物理学 · 物理学 2009-10-22 D. A. Frail , W. M. Goss , J. B. Z. Whiteoak

Type 1a supernova magnitudes conventionally include an additive parameter called the extinction coefficient. We find that the extinction coefficients of a popular ``gold'' set are well correlated with the deviation of magnitudes from Hubble…

天体物理学 · 物理学 2009-11-13 Pankaj Jain , John P. Ralston

Massive stars undergo a violent death when the supply of nuclear fuel in their cores is exhausted, resulting in a catastrophic "core-collapse" supernova. Such events are usually only detected at least a few days after the star has exploded.…

Astrophysical ionizing radiation events such as supernovae, gamma-ray bursts, and solar proton events have been recognized as a potential threat to life on Earth, primarily through depletion of stratospheric ozone and subsequent increase in…

地球与行星天体物理 · 物理学 2016-01-15 Brian C. Thomas , Byron D. Goracke

Gamma Ray Bursts as recent GRB990123 and GRB990510 are observed to occur in cosmic volumes with a corresponding output reaching, for isotropic explosions, energies as large as two solar masses annihilation. These energies are underestimated…

天体物理学 · 物理学 2007-05-23 Daniele Fargion