M83 从 GALEX UV 成像得到的消光径向轮廓
天体物理学
2009-11-10 v1
摘要
我们利用 GALEX 获取的 M83 的远紫外 (FUV) 和近紫外 (NUV) 图像，计算出星际形成盘中 UV 光谱斜率的径向轮廓。我们简要介绍了其化学演化模型，以获取星际暴露于的真实特性。使用衍生数据，我们还计算了 H-alpha/H-beta 和总红外 (TIR) 至 FUV 比值的轮廓。将数据和模型一起用于估计并比较由各种指示器获得的 FUV 波长处的消光梯度。我们讨论了对于星际形成率的确定的含义。
引用
@article{arxiv.astro-ph/0411375,
title = {Extinction radial profiles of M83 from GALEX UV imaging},
author = {S. Boissier and A. Gil de Paz and B. F. Madore and A. Boselli and V. Buat and D. Burgarella and P. G. Friedman and T. A. Barlow and L. Bianchi and Y. -I. Byun and J. Donas and K. Forster and T. M. Heckman and P. N. Jelinsky and Y. -W. Lee and R. F. Malina and D. C. Martin and B. Milliard and P. Morrissey and S. G. Neff and R. M. Rich and D. Schiminovich and O. H. W. Siegmund and T. Small and A. S. Szalay and Barry Y. Welsh and T. K. Wyder},
journal= {arXiv preprint arXiv:astro-ph/0411375},
year = {2009}
}
备注
This paper will be published as part of the Galaxy Evolution Explorer (GALEX) Astrophysical Journal Letters Special Issue. Links to the full set of papers will be available at http://www.galex.caltech.edu/PUBLICATIONS/ after November 22, 2004. A high resolution version of figure 1 is available at http://www.ociw.edu/~boissier/M83/fig1.ps