8 research outputs found

    The expansion field: The value of H_0

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    Any calibration of the present value of the Hubble constant requires recession velocities and distances of galaxies. While the conversion of observed velocities into true recession velocities has only a small effect on the result, the derivation of unbiased distances which rest on a solid zero point and cover a useful range of about 4-30 Mpc is crucial. A list of 279 such galaxy distances within v<2000 km/s is given which are derived from the tip of the red-giant branch (TRGB), from Cepheids, and from supernovae of type Ia (SNe Ia). Their random errors are not more than 0.15 mag as shown by intercomparison. They trace a linear expansion field within narrow margins from v=250 to at least 2000 km/s. Additional 62 distant SNe Ia confirm the linearity to at least 20,000 km/s. The dispersion about the Hubble line is dominated by random peculiar velocities, amounting locally to <100 km/s but increasing outwards. Due to the linearity of the expansion field the Hubble constant H_0 can be found at any distance >4.5 Mpc. RR Lyr star-calibrated TRGB distances of 78 galaxies above this limit give H_0=63.0+/-1.6 at an effective distance of 6 Mpc. They compensate the effect of peculiar motions by their large number. Support for this result comes from 28 independently calibrated Cepheids that give H_0=63.4+/-1.7 at 15 Mpc. This agrees also with the large-scale value of H_0=61.2+/-0.5 from the distant, Cepheid-calibrated SNe Ia. A mean value of H_0=62.3+/-1.3 is adopted. Because the value depends on two independent zero points of the distance scale its systematic error is estimated to be 6%. Typical errors of H_0 come from the use of a universal, yet unjustified P-L relation of Cepheids, the neglect of selection bias in magnitude-limited samples, or they are inherent to the adopted models.Comment: 44 pages, 4 figures, 6 tables, accepted for publication in the Astronony and Astrophysics Review 15

    Arthur Robert Hogg

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    Note on Band Transmission in Multilayer Dielectric Filters

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    The existence of pass and stop bands for periodically stratified media, in particular for multilayer dielectric filters, is well known, but there seems to be no way of demonstrating this either without the use of a good deal of algebra or by appeal to relatively unfamiliar ideas, such as those of transmission line theory. Our purpose here is to show that for an infinite medium, this result can be established by a direct adaptation of the Kronig-Penney (1931) model for metal lattices. Accounts of this model are given in a number of textbooks (Rojansky 1942; Brillouin 1946) and also in undergraduate courses in this country, so that it may be considered well known. Mathematical details will accordingly be abbreviated; they may be found in the references cited.</jats:p

    Przybylski, Antoni

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    Ellery, Robert Lewis John

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    The Theory of Galactic Rotation

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