The proceedings will be published in New Astronomy Reviews (New Astronomy Reviews at Science Direct) of Elsevier Science publishers. This journal is listed in ISI. All contributions will be peer reviewed and edited for content and style. The papers are going to be reviewed by a member of the SOC and a participant of the school in order to increase the quality of the proceedings.
The deadline for submission of manuscripts in PDF format is September 4, 2007. Please send your manuscript to porto-editors@mpia.de.
Manuscripts must be prepared according to the instructions given below. Further information on general instructions to authors from this journal may be found on the Elsevier’s Author Gateway web pages.
Instructions
Manuscripts should preferably be prepared in LaTeX using Elsevier’s manuscript preparation style "elsart". The "elsart" style files as well as a description on their use can also be found on Elsevier’s Author Gateway. It can be retrieved by anonymous ftp from one of these mirrors of the Internet Comprehensive TEX Archive: UK mirror, Germany mirror, USA mirror.
- Chapter 1-4: 25-30 pages (Lodato, Ferreira, Alexander, Klahr, Akeson, Testi/Leurini, Duchene/Augereau, Wood, Santos, Hummel)
- Chapter 5: 10-15 pages (Millour, Percheron, Hummel, Delplancke)
- The LaTeX file of your contribution(s)
- Separate files for any diagrams or images (please make sure that they complish with Elsevier’s artwork standards)
- A postscript file of the article in its final form.
The postscript file is for reference purposes only and will serve to ensure that all the matter pertaining to the contribution has been received by the editors.
Please note...
- Don’t alter the basic New Astronomy Reviews format regarding line spacing, indentation, etc., as set out in the LaTeX style file.
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- An abstract up to about 150 words must be supplied.
- Place your illustrations and tables inside the text body and provide captions for all of them.
- References in the text are indicated by name and date, and the full reference should be given in an alphabetical list at the end of the paper.
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The book lay-out follows this outline
- Foreword (Wolf/Garcia)
- Interferometry in the context of star/planet formation
- Interferometry in the context of star/planet formation
- Circumstellar Disk Structure and Evolution
- Classical disks physics (Lodato)
- Magnetized disks (Ferreira)
- Planet Formation in Disks
- From disks to planetesimals I - Gas and dust evolution (Alexander)
- From disks to planetesimals II - Disk-planet interaction (Klahr)
- Observations of Protoplanetary Disks and Planets
- Optical interferometric observations of disks (Akeson)
- Millimeter interferometry of disks (Testi/Leurini)
- HST/AO and coronography of disks and planets (Duchéne/Augereau)
- Modeling Circumstellar Disks (Wood)
- Planet searching techniques (Santos)
- Interferometric Data Processing (Hummel)
- Interferometry in Practice
- Visibility and Visibility Models (Millour)
- UV space and observability (Millour)
- Calibrators (Percheron)
- Processing of MIDI and AMBER data (Hummel)
- The PRIMA instrument (Delplancke)
- Sumary and future directions (Garcia/Wolf)
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