Zobrazeno 1 - 10
of 34
pro vyhledávání: '"D. S. Hayes"'
Autor:
D. Mameri, D. S. Hayes, S. Führer, E. Fauchery, S. Schmutz, A. Monserat, T. Hasler, D. R. M. Graf, J. M. Santos, M. T. Ferreira, S. Auer
Publikováno v:
Aquatic Sciences. 85
Research on how intermittent water releases from hydropower plants affect the early life stages of fish has advanced in the last years, focusing not only on the direct impacts of rapid flow changes (hydropeaking), but also on the short-term fluctuati
Autor:
D. S. Hayes
Publikováno v:
Highlights of Astronomy. 7:819-826
Observed stellar energy distributions are used in synthetic photometry to evaluate the accuracy of the response functions and to determine the transformation coefficients. The characteristics required of a catalog of energy distributions to be used f
Autor:
D. S. Hayes, A. G. Davis Philip
Publikováno v:
Symposium - International Astronomical Union. 111:469-472
The energy distributions of 16 horizontal-branch A-stars and 11 horizontal-branch stars in globular clusters have been measured using the Harvard Scanners at KPNO and CTIO and the Oke multichannel spectrophotometer on the 5-m telescope at Mt. Palomar
Autor:
D. S. Hayes
Publikováno v:
Symposium - International Astronomical Union. 111:225-252
The absolute fluxes and energy distributions of stars are the foundation of the calibration of fundamental effective temperatures and bolometric corrections. In this paper I will review recent progress in the calibration of absolute fluxes and energy
Publikováno v:
Astrophysics and Space Science. 112:251-257
Photoelectric Vilnius photometry of the B-type stars HD 29 647 and HDE 283 809 in the direction of the Taurus molecular cloud indicates their brightness and energy distribution to be constant within 1–2%. The interstellar extinction law is determin
Autor:
D. S. Hayes
Publikováno v:
Symposium - International Astronomical Union. 80:65-76
Scales of fundamental bolometric connections (B.C.) and effective temperatures (Teff) as a function of spectral type or color are necessary for the comparison of observations and theory in the HR diagram.
Publikováno v:
Symposium - International Astronomical Union. 52:83-90
We have analysed observations of the interstellar extinction in the range 3400 Å–l 1000 Å. The observations have high photometric accuracy and wavelength resolution, and allow a detailed examination of broadband structure as well as the general s
Publikováno v:
Symposium - International Astronomical Union. 105:171-173
Studies are underway concerning the masses of horizontal-branch A stars. Hayes and Philip (1979) discussed masses determined for seven field HB stars using gravities and temperatures obtained from spectrophotometric scans. They found a mean mass of 0
Autor:
D. S. Hayes
Publikováno v:
The HR Diagram ISBN: 9789027709066
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d003146a7b3c90b215d12e9b13af3fde
https://doi.org/10.1007/978-94-009-9851-3_14
https://doi.org/10.1007/978-94-009-9851-3_14
Publikováno v:
Observational Tests of the Stellar Evolution Theory ISBN: 9789027717757
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cc565264f55e3d3be2a2efdbb47aff06
https://doi.org/10.1007/978-94-010-9570-9_30
https://doi.org/10.1007/978-94-010-9570-9_30