Related records
Services
-
Articles citing this article
-
Same authors
- Recommend this article
- Download citation
- Alert me if this article is cited
- Alert me if this article is corrected
|
||||||||||||||||||
A&A 478, 795-795 (2008)
DOI: 10.1051/0004-6361:20078536e
Erratum
A search for near-infrared molecular hydrogen emission in the CTTS LkH
264 and the debris disk 49 Ceti
A. Carmona1, 2, M. E. van den Ancker2, Th. Henning1, M. Goto1, D. Fedele2, 3, and B. Stecklum4 1 Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
e-mail: carmona@mpia.de
2 European Southern Observatory, Karl Schwarzschild Strasse 2, 85748 Garching bei München, Germany
3 Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
4 Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany
Without abstract
Key words: stars: emission-line, Be -- stars: pre-main sequence -- planetary systems: protoplanetary disks -- errata, addenda
© ESO 2008
| 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.

BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook