Measurement of the stellar irradiance f - inaoe
Measurement of the stellar irradiance f - inaoe Measurement of the stellar irradiance f - inaoe
Some results The theoretical U-B versus B-V diagram is plotted for log g=4.0 and 4.5 for and for log g=4.5 and 5.0 for (crosses). It is compared with the observed unreddened dwarf locus. (Bessell , 1998, A&A, 333, 231)
What is measured ? Heterochromatic magnitude
- Page 1: Measurement of the stellar irradian
- Page 5 and 6: Some basic notations : (R = radius
- Page 7 and 8: Energy received at Earth : (stellar
- Page 9 and 10: monochromatic magnitude of Vega (Ok
- Page 11 and 12: Cohen et al.1992, AJ, 104, 1650
- Page 13 and 14: Ratio of the final STIS fluxes for
- Page 15 and 16: Comparison as in Fig. 6 for the Bal
- Page 17 and 18: Catalogues of SED Jacoby et al, 198
- Page 19 and 20: Some results uvby photometry : Comp
- Page 21: Zero-point of synthetic photometric
- Page 28 and 29: Heterochromatic extinction : effect
- Page 30 and 31: A(λ=V) R = -------------------- E(
- Page 32 and 33: ( from: B. Chen at al A&A 336, 137,
Some results<br />
The <strong>the</strong>oretical U-B versus B-V<br />
diagram is plotted for log g=4.0<br />
and 4.5 for and for log g=4.5<br />
and 5.0 for (crosses). It is<br />
compared with <strong>the</strong> observed<br />
unreddened dwarf locus.<br />
(Bessell , 1998, A&A, 333, 231)
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