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The formation of the first stars and galaxies

supernovae (PISNe), which disrupt the entire – 13 – REFERENCES 1 Barkana, R. Loeb, matter (WDM) simulations (right) at z = 20

The Relative Specific Type Ia Supernovae Rate From Three

Supernova (ASAS-SN) Bright Supernova Catalogs to determine the observed where it is enhanced by a factor of $\sim10-20$ relative to host

Fhit modulation of the Akt-survivin pathway in lung cancer

20 OAS1 FRS2 ATXN1 ULBP2 COL1A1 LY96 JMY pAdenoVator-CMV5-GFP (Qbiogene, Carlsbad, CA,Ottey M, Han SY, Druck T, Barnoski BL, Mc

Exposure to carbon nanotube material: assessment of nanotube

J Toxicol Environ Health A. 2003 Oct 24;66(20):1909-26. 2003 Oct 24;66(20):1909-26. Exposure Shvedova AA1, Castranova V, Kisin ER,

Toxicity of lunar dust assessed in inhalation-exposed rats

Castranova V, Driscoll KE, Gardner DE, McClellan RO, Cooper BL, McKay 20.8 and 60.6 mg/m(3) of respirable-size lunar dust for 4 weeks

New cosmological mass limit on thermal relic axions

[Supernova Search Team Collaboration], Type Ia [43] A. Goobar, E. Mo¨rtsell, R. Ama 20 (2002) [astro-ph/0012324]. [45] N. Y

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atomic and molecular gas in the vicinity of the supernova

gas in the vicinity of the supernova remnant the emission is accelerated by about 20 km/s. bar is surrounded by a region of enhanced

Simulating the detection and classification of

spaxel scale, we can classify supernova Type Ia and their redshift robustly up to 80 days past maximum light (20 days in the supernova rest frame)

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observations of type IIn supernovae: typical properties

20 days) followed by a slow decline stage (supernovae (SNe; Minkowski 1941; see FilippenkoNorth is up, East is due left, a scale bar

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Optical Imaging and Spectroscopy of the Galactic Supernova

Fig. 20.—Distribution plot of 3C 58 knots showing low negative radial supernova. The remnants PWN is also too large to have expanded in just

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supernovae : general turbulenceIn this paper, we study the role of superThe latter can reach 20% for isolated bubbles, but on average it does

Neutrino emission from type II supernovae - an analysis of

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