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Numerical Hydrodynamics in General Relativity. [PDF]
Font JA.
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Numerical Hydrodynamics and Magnetohydrodynamics in General Relativity. [PDF]
Font JA.
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Gravitational Lensing in Astronomy. [PDF]
Wambsganss J.
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Cosmological implications of light element abundances: theory. [PDF]
Schramm DN.
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A binary merger product as the direct progenitor of a Type II-P supernova
Niu* Z +17 more
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Causes and effects of the first quasars. [PDF]
Rees MJ.
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2017
In this chapter presents supernovae of Type Ib (SN Ib), the distinguishing characteristic of which is presence of helium spectral lines in optical spectra. Hydrogen lines are absent or inconspicuous, indicating that most or all of the hydrogen envelope was lost prior to explosion.
David Branch, J. Craig Wheeler
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In this chapter presents supernovae of Type Ib (SN Ib), the distinguishing characteristic of which is presence of helium spectral lines in optical spectra. Hydrogen lines are absent or inconspicuous, indicating that most or all of the hydrogen envelope was lost prior to explosion.
David Branch, J. Craig Wheeler
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The X-ray Emission of Type Ib∕c Supernovae
AIP Conference Proceedings, 2007Before the launch of Chandra and XMM‐Newton, only two type Ib/c supernovae had been observed in X‐rays (1994I and 1998bw). I will review briefly the advances of the past seven years in the early (days to weeks) X‐ray detection of type Ib/c supernovae, a recent effort to characterize the X‐ray emission of years‐old Ib/c supernovae (e.g., 2001em, 2003bg,
D. Pooley, Stefan Immler, Kurt Weiler
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Supernova 1993J as a spectroscopic link between type II and type Ib supernovae
Nature, 1993Supernova 1993J in the nearby galaxy M81 is one of the closest - and hence brightest - supernovae to be witnessed this century. The early spectrum of SN1993J showed the characteristic hydrogen signature of type II supernovae, but its subsequent evolution is atypical for this class of supernova. Here we present optical and infrared spectra of SN1993J up
D. A. Swartz +4 more
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On the Nature of Type Ib Supernova Progenitors
1991The realization that there is a separate subclass of Type I supernovae (SNe) to be denoted as Type Ib came after the detailed study of the SN 1983N in M83 (PANAGIA et al [1]; see also PANAGIA [2], WHEELER and LEVREAULT [3], UOMOTO and KIRSHNER [4]). It was immediately clear that SN 1983N is distinctly different from the classical variety of Type I SNe (
Nino Panagia, Victoria G. Laidler
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