Zobrazeno 1 - 10
of 13
pro vyhledávání: '"D. J. I. Fry"'
Publikováno v:
Publications of the Astronomical Society of the Pacific. 110:433-450
This is the third in a series of papers on large-amplitude δ Scuti and related stars intended to determine Baade-Wesselink radii and luminosities with precision. The first two papers discussed our method of analysis and its application to the δ Scu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a3912bee40f065e8d63c9e5a603b07ad
https://doi.org/10.1086/316148
https://doi.org/10.1086/316148
Publikováno v:
Publications of the Astronomical Society of the Pacific. 106:1120
This is the second paper in a series on large-amplitude delta Scuti stars intended to determine Baade-Wesselink radii and luminosities with precision. The first paper discussed our method of analysis and its application to EH Librae; in this paper we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d7894d2143ca27805a0f2075480e1cf4
https://doi.org/10.1086/133488
https://doi.org/10.1086/133488
Publikováno v:
Publications of the Astronomical Society of the Pacific. 106:550
This is the first of a short series of papers on large-amplitude delta Scuti variables. The determination of Baade-Wesselink radii and luminosities for pulsating stars is a long-standing and highly desired goal since such quantiites provide necessary
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b1454efca4424c01e41bab0b00d37740
https://doi.org/10.1086/133414
https://doi.org/10.1086/133414
Publikováno v:
Publications of the Astronomical Society of the Pacific. 105:809
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e3502c3fbe159213d9d0bd809d984da8
https://doi.org/10.1086/133237
https://doi.org/10.1086/133237
Publikováno v:
International Astronomical Union Colloquium. 139:104-104
The determination of Baade-Wesselink radii and luminosities for pulsating stars are long-standing and highly desired goals since they provide the promise of being standard candles. In a modest contribution towards these goals, we have undertaken a pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d978af81f4183bcd41181fc999512f53
https://doi.org/10.1017/s0252921100117026
https://doi.org/10.1017/s0252921100117026
Publikováno v:
The Astrophysical Journal. 370:677
Observations and analyses of the binary TY Bootis are presented. Radial velocity data are used for the first time to establish the mass ratio without ambiguity, and an advanced version of the Wilson-Devinney synthetic light curve program is used to a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::acdae15e224ec27067f3fd04b1c807f6
https://doi.org/10.1086/169852
https://doi.org/10.1086/169852
Publikováno v:
Celestial Mechanics. 45:135-139
A major program at the University of Calgary's Rothney Astrophysical Observatory (RAO) is the study of eclipsing close-binary stars, which, because of circularization effects, are all cases of the restricted three-body problem. The physical propertie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dc4f4a648b3aefbdf227bc1bd3328d67
https://doi.org/10.1007/bf01228994
https://doi.org/10.1007/bf01228994
Publikováno v:
Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences. 266:84-94
Electron nuclear double resonance has been carried out in single crystals of MgO containing Co 2± . An accurate check of the spin-Hamiltonian has been made and the relevant parameters measured as A = 290.55 ± 0.06 Mc/s, g' N β N /gβ = 2.34 ± 0.0
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::40635d07b5719057d76faffe2e715201
https://doi.org/10.1098/rspa.1962.0048
https://doi.org/10.1098/rspa.1962.0048
Publikováno v:
Applications of Computer Technology to Dynamical Astronomy ISBN: 9789401069328
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b64200399dfa20884e368601c1efb207
https://doi.org/10.1007/978-94-009-0985-4_26
https://doi.org/10.1007/978-94-009-0985-4_26
Publikováno v:
Late Stages of Stellar Evolution ISBN: 9789401081962
Subsequent to the discovery of a radio flare in CH Cyg (Taylor, Seaquist, and Mattei 1986), bolometer (JHKLMNQ and 12.8 m) observations carried out in June 1985 have been combined with optical (UBVRI) data from May and July 1985 to produce a broadban
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d1b0f06338d04f03b59dc21064920df8
https://doi.org/10.1007/978-94-009-3813-7_45
https://doi.org/10.1007/978-94-009-3813-7_45