Effective temperatures by Infrared Flux Method (Blackwell+ 1998)

Details Effective temperatures by Infrared Flux Method (Blackwell+ 1998) Effective temperatures by Infrared Flux Method (Blackwell+ 1998)

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ycat..41290505b&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/129/505. Originally published in: 1998A&AS..129..505B

Physics

Effective Temperatures, Photometry: Infrared

Scientific paper

Effective temperatures for 420 stars with spectral types between A0 and K3, and luminosity classes between II and V, selected for a flux calibration of the Infrared Space Observatory, ISO, have been determined using the Infrared Flux Method (IRFM). The determinations are based on narrow and wide band photometric data obtained for this purpose, and take into account previously published narrow-band measures of temperature.
(1 data file).

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