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A review of the distance and structure of the Large Magellanic Cloud
DOI: 10.1016/j.newar.2004.03.001 Bibcode: 2004NewAR..48..659A

Alves, David R.

The average of 14 recent measurements of the distance to the Large Magellanic Cloud (LMC) implies a true modulus of 18.50 ± 0.02 mag, and demonstrates a trend in the past 2 years of convergence toward a standard value. The distance indicators reviewed are the red clump, the tip of the red giant branch, Cepheid, RR Lyrae, and Mira variable stars, c…

2004 New Astronomy Reviews
eHST 130
Elemental composition and distribution in SNRs: X-ray spectroscopy
DOI: 10.1016/j.newar.2003.11.010 Bibcode: 2004NewAR..48...75D

Decourchelle, A.

I present a comparative review focusing on three young Supernova Remnants, Cas A, Tycho and Kepler, in the light of recent X-ray observations obtained with the XMM-Newton and Chandra satellites. Recently available, X-ray spectro-imagery of young Supernova Remnants is providing unique information on the interaction region between the ejected materi…

2004 New Astronomy Reviews
XMM-Newton 2
Dust production in supernovae
DOI: 10.1016/j.newar.2003.12.052 Bibcode: 2004NewAR..48..611D

Dunne, L.; Eales, S.; Ivison, R. +2 more

The question `Are supernovae important sources of dust?' is a contentious one. Condensation theory and observations of dust at very high redshifts suggests that they should be, since only massive stars evolve quickly enough to produce the large quantities of dust seen at such early times in the Universe. However, observations with IRAS and ISO hav…

2004 New Astronomy Reviews
ISO 2