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We also find that infrared dust emission may be detectable in typical superluminous supernovae out to $\sim$ 100-1000 Mpc in 2-5 years after the

How a Star Cluster Ruled Out MACHOs

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Vela as the Source of Galactic Cosmic Rays above 100 TeV

Vela as the Source of Galactic Cosmic Rays above 100 TeV Abstract: We model the contribution of the nearest young supernova remannt Vela to the local

Vela as the Source of Galactic Cosmic Rays above 100 TeV

Vela as the Source of Galactic Cosmic Rays above 100 TeV Abstract: We model the contribution of the nearest young supernova remannt Vela to the local

in the High-Entropy Wind of Core-Collapse Supernovae

Co-Production of Light and Heavy p-, s- and r-Process Isotopes in the High-Entropy Wind of Core-Collapse Supernovae doi:10.22323/1.100.008111th

Geysers from the Tiger Stripes of Enceladus

material in Saturns E ring, in which Enceladus ~100 geysers coming from the tiger stripes in //aasnova.org/wp-content/uploads/2015/10/PIA

acceleration above 100 TeV in the shell-type Supernova

Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7-3946 with deep H.E.S.S. observations

Stress heterogeneity in siltstone using synchrotron x-ray

siltstone ( 65% quartz) with reference sample novaculite (100% quartz). geomaterial, and hence, it is important to understand both the heterogeneity

Are LIGOs Black Holes Made From Smaller Black Holes?

100 LIGO detections, we should be able to tell whether these black holes 《Aas Nova Highlights》Fishbach, M., D. Holz, and B. Farr (2017)

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Center electrode material NiY Centre electrode 2,7 mm Designation Spark Type of connection Detachable DIN/SAE nut Width across flats 20,8 mm

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Chandra Observations of ``The Antennae Galaxies (NGC 4038/

(X-ray binaries, XRBs, and supernova rem- nants [SNRs]), as well asAt a distance of 29 Mpc, 100 corresponds to a physical distance of 140

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Gamma-Ray Observations of Supernova Remnants

Gamma-Ray Observations of Supernova RemnantsDespite the growing evidence for However, 200 GeV to 100 TeV measurements revealed no significant emission

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NICER Eyes on Bursting Stars

in which a compact object accretes material And, as there are over 100 such X-ray bursterKohler, Susanna《Aas Nova Highlights》

Differential expression of iron-, carbon-, and oxygen-

Manga- nelli, R., Chan, W.T., Tsenova, L., Gold, B., Smith, P Natl Acad Sci USA 100 : 14321 – 14326

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from 10–100 TeV Cosmic‐Ray Electrons in the Supernova

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Abstract: Tychos supernova remnant (SNR) has a periphery which clearly {-1}$, a pole velocity of $\sim 100$~km s$^{-1}$, a duration

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acceleration above 100 TeV in the shell-type Supernova

Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7-3946 with deep H.E.S.S. observations

Probing the Interstellar Medium near Star-forming Regions

its molecular cloud or circumstellar material). supernovae have been identified at the same hundred Myr (Calura et al. 2003; Dessauges-

Extraterrestrial cause for the cretaceous-tertiary extinction

average patterns expected for crustal material (46100 million years, a supernova occurred within Flex- ser and M. Sturz of Lawrence Berkeley