THE NATURE AND EVOLUTION OF DISKS AROUND HOT STARS

	Instructions for Contributions to the Proceedings
	-------------------------------------------------


The proceedings are to be published by the Astronomical Society of the
Pacific (ASP) in their conference series.  Editors will be Richard Ignace
and Kenneth Gayley.  The following provides instructions for submission
of contributions for the proceedings.


* Contributions are due by September 1st

* The style file for the ASP and instructions can be found at

      www.astrosociety.org/pubs/cs/confseries.html

  Click on the 'Authors Macros' along the lefthand menu.

* Page limit reminder:  

     Review Talks - 12 pages
     Focus Sessions - 12 pages
     Discussion Sessions - 12 pages
     Posters - 4 pages

* We anticipate having author, object, and subjectindices.  To aid in 
  producing these, please adhere to the following.

  Following the '\end{document}' line of your contribution, use the following
  format to recommend entries for these indices (best described with examples):

  AWORD for authors

  OWORD for objects

  SWORD for subject key words

  Example -

  ... text of latex file ...
  \end{document}

  AWORD: Happy, I. B.
  AWORD: Sleepy, I. M.
  AWORD: Smart, I. R.
  
  OWORD: $\zeta$ Pup
  OWORD: mega Oph
  OWORD: NGC 0000

  SWORD: nonsense
  SWORD: Nobel Prize
  SWORD: imagination, main results
  SWORD: error analysis, plotting confidence guesses 


  The goal here is to be able to run standard unix stream editing functions
  to produce more easily the indices, as for example

     grep AWORD *.tex | awk '{ printf("\\indexentry{") for (i=2;i<=NF;i++) 
                                      { printf("%s ", $i) } printf("}\n") } '

        (Or something like this.  Everything runs in unix, if it has 
         enough slashes and such.  Just might not be what you want.   :)


  Please limit the number of suggested keywords for the subject index
  to 5 entries for your contribution.

* Finally, when submitting your contribution, please send a single gzipped
  tar file containing your latex file and eps figures using the following
  format:

  Jones_A.tex
  Jones_A.f1.eps
  Jones_A.f2.eps
  ...

  so that all files begin with the last name, followed by an underscore,
  followed by a first initial for the lead author.  Similar for the eps
  figure files.

  Then to create the gzipped tar file, type

     tar -cvzf Jones_A.tar.gz Jones_A*

  Email the file Jones_A.tar.gz to hotstars@etsu.edu (NOT to the ignace
  or to the kgg email, please).

* Final Comments:  No color figures will be published.  Half-tones are
  acceptable.  If you have a color figure that you want to appear as
  grayscale, you should re-render the figure as grayscale specifically.
  The ASP warns that for example red and blue in a color figure when
  printed in black and white appear as the same shade, and yellow is
  essentially white.  Further, avoid referring to figure colors in text
  body or caption, as this will be confusing.



If you have any questions about contributions to the proceedings, feel free
to contact the editors at ignace@etsu.edu and/or kgg@astro.physics.uiowa.edu.

Thank you.





Best Regards,

Rico Ignace
Ken Gayley