EDP Sciences Journals List
Advanced Search

Free access article

Issue A&A
Volume 456, Number 3, September IV 2006
Page(s) 967 - 967
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20053933e



A&A 456, 967-967 (2006)
DOI: 10.1051/0004-6361:20053933e

AGB stars in the Magellanic Clouds

II. The rate of star formation across the LMC
M.-R. L. Cioni1, L. Girardi2, P. Marigo3 and H. J. Habing4

1  SUPA, School of Physics, University of Edinburgh, IfA, Blackford Hill, Edinburgh EH9 3HJ, UK
    e-mail: mrc@roe.ac.uk
2  Osservatorio Astronomico di Trieste, INAF, via G. B. Tiepolo 11, 34131 Trieste, Italy
3  Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
4  Sterrewacht Leiden, Niels Bohrweg 2, 2333 RA Leiden, The Netherlands

( A&A 448, 77-91 (2006), DOI: 10.1051/0004-6361:20053933 )

Abstract


Key words: galaxies: Magellanic Clouds -- stars: late-type -- Galaxy: abundances -- stars: luminosity function, mass function -- errata, addenda



© ESO 2006

What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.