Changes between Version 64 and Version 65 of StellarAtmospheres


Ignore:
Timestamp:
2020-02-04T19:54:15Z (2 months ago)
Author:
Gary J. Ferland
Comment:

update tlusty web site

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  • StellarAtmospheres

    v64 v65  
    246246== Tlusty O and B star grids ==
    247247
    248 [http://nova.astro.umd.edu/Tlusty2002/tlusty-frames-cloudy.html Tlusty SEDs for Cloudy][[BR]]
    249 
    250 The [http://nova.astro.umd.edu/ Tlusty] code is maintained by Ivan Hubeny & Thierry Lanz.  They have produced extensive grids of non-LTE, line-blanketed, plane-parallel, hydrostatic O and B star SEDs. The [http://nova.astro.umd.edu/Tlusty2002/tlusty-frames-cloudy.html ''SEDs for Cloudy''] link on their main web site gives links to the files we use.
    251 
    252 There are 11 sets of O star SEDs compiled from the [http://nova.astro.umd.edu/Tlusty2002/tlusty-frames-OS02.html OSTAR2002 grid] with names "ostar2002_*.ascii.gz". They are described in the reference [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?2003ApJS..146..417L&db_key=AST Lanz, T., & Hubeny, I. 2003, ApJS, 146, 417].  These SEDs are used by the ''stars_ostar2002*.in'' simulations in the test suite.
    253 
    254 At the time of this writing the B star grid is still under construction. There are currently 7 sets of B star SEDs compiled from the [http://nova.astro.umd.edu/Tlusty2002/tlusty-frames-BS06.html BSTAR2006 grid] with names ''bstar2006_*.ascii.gz''. They are described in the reference [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2007ApJS..169...83L&db_key=AST&data_type=HTML&format=&high=45d30ec84024291 Lanz, T., & Hubeny, I. 2007, ApJS, 169, 83]. These SEDs are used by the ''stars_bstar2006*.in'' simulations in the test suite.
     248[http://tlusty.oca.eu/Tlusty2002/tlusty-frames-cloudy.html Tlusty SEDs for Cloudy][[BR]]
     249
     250The [http://tlusty.oca.eu/ Tlusty] code is maintained by Ivan Hubeny & Thierry Lanz.  They have produced extensive grids of non-LTE, line-blanketed, plane-parallel, hydrostatic O and B star SEDs. The [http://tlusty.oca.eu/Tlusty2002/tlusty-frames-cloudy.html ''SEDs for Cloudy''] link on their main web site gives links to the files we use.
     251
     252There are 11 sets of O star SEDs compiled from the [http://tlusty.oca.eu/Tlusty2002/tlusty-frames-OS02.html OSTAR2002 grid] with names "ostar2002_*.ascii.gz". They are described in the reference [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?2003ApJS..146..417L&db_key=AST Lanz, T., & Hubeny, I. 2003, ApJS, 146, 417].  These SEDs are used by the ''stars_ostar2002*.in'' simulations in the test suite.
     253
     254At the time of this writing the B star grid is still under construction. There are currently 7 sets of B star SEDs compiled from the [http://tlusty.oca.eu/Tlusty2002/tlusty-frames-BS06.html BSTAR2006 grid] with names ''bstar2006_*.ascii.gz''. They are described in the reference [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2007ApJS..169...83L&db_key=AST&data_type=HTML&format=&high=45d30ec84024291 Lanz, T., & Hubeny, I. 2007, ApJS, 169, 83]. These SEDs are used by the ''stars_bstar2006*.in'' simulations in the test suite.
    255255
    256256Starting with the C10 release of Cloudy, we have added support for merged OSTAR2002/BSTAR2006 grids. The resulting grids have a temperature coverage from 15 to 55 kK. In the overlap region between 27.5 and 30 kK, the BSTAR2006 models have been adopted. The merged grids have been produced for all metallicities supported by the BSTAR2006 grid. They have names ''obstar_merged_*.ascii.gz''. When you use one of these grids, you should cite both [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?2003ApJS..146..417L&db_key=AST Lanz, T., & Hubeny, I. 2003, ApJS, 146, 417] and [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2007ApJS..169...83L&db_key=AST&data_type=HTML&format=&high=45d30ec84024291 Lanz, T., & Hubeny, I. 2007, ApJS, 169, 83]. These SEDs are used by the ''stars_obstar_merged*.in'' simulations in the test suite.