Luminosity Function for weak part main sequence.

Details Luminosity Function for weak part main sequence. Luminosity Function for weak part main sequence.

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998larm.confe..40p&link_type=abstract

"IX Latin American Regional IAU Meeting, "Focal Points in Latin American Astronomy", held in Tonantzintla, Mexico, Nov 9-13, 199

Astronomy and Astrophysics

Astronomy

Scientific paper

In this analysis, the objetive is obtain the Luminosoty Function for stars within main sequence and certain criteria selection. I used stars than meet following the criteria: one, That here a visual magnitude larger than 5, and second, stars whose "parallax relative error" < 0.2. This stars are in both cataloges; Hipparco (118,222 stars) and Tycho (1,058,222 stars).

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