Results 181 to 190 of about 7,219,823 (215)

Gravitational Lensing in Astronomy. [PDF]

open access: yesLiving Rev Relativ, 1998
Wambsganss J.
europepmc   +1 more source

A binary merger product as the direct progenitor of a Type II-P supernova

open access: yes
Niu* Z   +17 more
europepmc   +1 more source

Causes and effects of the first quasars. [PDF]

open access: yesProc Natl Acad Sci U S A, 1993
Rees MJ.
europepmc   +1 more source

Type Ib Supernovae

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
openaire   +1 more source

The X-ray Emission of Type Ib∕c Supernovae

AIP Conference Proceedings, 2007
Before 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
openaire   +1 more source

Supernova 1993J as a spectroscopic link between type II and type Ib supernovae

Nature, 1993
Supernova 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
openaire   +1 more source

On the Nature of Type Ib Supernova Progenitors

1991
The 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
openaire   +1 more source

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