DRIFT-PHOENIX models Virtual Observatory Resource

Authors

1. Woitke P., Helling C., 2003, A&A, 399, 297

Published by

SVO CAB

Abstract

Drift-Phoenix is a computer code that simulates the structure of an atmosphere including the formation of clouds. The code is part of the Phoenix-code family. Drift describes the formation of mineral clouds and allows to predict cloud details, like the size of the cloud particles and their composition.

Keywords

1. star

Bibliographic source HTTP

http://adsabs.harvard.edu/abs/2003A%26A...399..297W

See also HTML

http://svo.cab.inta-csic.es/

IVOA Identifier IVOID

ivo://svo.cab/models/drift

Access

IVOA Simple Spectrum Search SSAP

For use with a VO-enabled spectral analysis program (e.g., Splat, VOSpec).
http://svo2.cab.inta-csic.es/theory/newov2/ssap.php?model=drift&