Results 191 to 200 of about 21,733 (235)
<i>In situ</i> analysis of titanium isotope ratios in stardust using LA-CC-MC-ICPMS/MS. [PDF]
Shaw KMM +6 more
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Multiple outflows and delayed ejections revealed by early imaging of novae. [PDF]
Aydi E +41 more
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Electromagnetic follow-up of gravitational waves: review and lessons learned. [PDF]
Nicholl M, Andreoni I.
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Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
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Determination of the mass distribution of the first stars from the 21-cm signal. [PDF]
Gessey-Jones T +8 more
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SALT2: using distant supernovae to improve the use of type Ia supernovae as distance indicators [PDF]
Aims. We present an empirical model of type la supernovae spectro-photometric evolution with time. Methods. The model is built using a large data set including light-curves and spectra of both nearby and distant supernovae, the latter being observed by ...
Mark Sullivan +2 more
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Is the Supernova 1950E a Supernova?
Publications of the Astronomical Society of Japan, 1990Abstract The supernova (SN) 1950E in the galaxy Zw 065.001 was found by Chai and van den Bergh (1970; AAA 04.125.005) on Palomar Observatory Sky Survey (POSS) plates. We have measured its position accurately and have found that the position on the blue print of POSS is different by about 3″ from that on the red print.
Tomohiro Ohsawa +2 more
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Superluminous Supernovae [PDF]
45 pages, 6 figures, a refereed review article to be published in Space Science ...
Takashi Moriya +2 more
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Supernovae and Supernova Remnants
1983Supernovae are the result of explosions which terminate the life of massive stars. The amount of energy released by the supernovae in our galaxy is so large that these explosions provide the dominant energy for the heating of the hot (T ≳ 106 K) IS component and for the kinetic energy of the large scale motions of the interstellar clouds.
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