Extinction by grey dust in the intergalactic medium
天体物理学
2007-05-23 v1
摘要
Condensation in the outer regions of decaying supernovae is an efficient source of dust with grain size up to 1 micron. The largest grains leave the parent galaxy, thus forming "grey" intergalactic dust, which can explain the observed dimming of light from distant supernovae without invoking cosmic acceleration
引用
@article{arxiv.astro-ph/0306459,
title = {Extinction by grey dust in the intergalactic medium},
author = {Ernst Fischer},
journal= {arXiv preprint arXiv:astro-ph/0306459},
year = {2007}
}
备注
6 pages