Statistics – Applications
Scientific paper
Feb 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aj....107..742g&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 107, no. 2, p. 742-746
Statistics
Applications
150
Atmospheric Models, Calibrating, Classifications, Dwarf Stars, Standards, Stellar Atmospheres, Stellar Models, Stellar Spectra, Stellar Temperature, Visible Spectrum, Applications Programs (Computers), Astronomical Spectroscopy, Charge Coupled Devices, Ibm Personal Computers, Light (Visible Radiation), Spectrographs, Stellar Gravitation
Scientific paper
Synthetic spectra based on the new Kurucz models and calculated using the International Business Machines (IBM) personal computer (PC)-based program SPECTRUM (which is described and made available to the astronomical community) are classified using the techniques of MK spectra classification against digital spectra of MK standards. The results are used to calibrate the MK system for solar-composition dwarf stars from B1 V to K5 V in terms of effective temperature.
Corbally Christopher J.
Gray Richard O.
No associations
LandOfFree
The calibration of MK spectral classes using spectral synthesis. 1: The effective temperature calibration of dwarf stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The calibration of MK spectral classes using spectral synthesis. 1: The effective temperature calibration of dwarf stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The calibration of MK spectral classes using spectral synthesis. 1: The effective temperature calibration of dwarf stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1013656