Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Tyler E. Nordgren"'
Publikováno v:
The Astrophysical Journal. 612:463-471
An asymmetric surface brightness distribution of the rapidly rotating A7IV-V star, Altair, has been measured by the Navy Prototype Optical Interferometer (NPOI). The observations were recorded simultaneously using a triangle of three long baselines o
Publikováno v:
NASA Astrophysics Data System
We present the period-radius relations predicted by nonlinear convective models of Classical Cepheids and RR Lyrae stars. For the former variables we show that the metallicity effect is negligible for both fundamental and first overtone pulsators. Th
Autor:
Massimo Marengo, Margarita Karovska, Dimitar D. Sasselov, Costas Papaliolios, John T. Armstrong, Tyler E. Nordgren
Publikováno v:
The Astrophysical Journal. 589:968-975
The geometric Baade-Wesselink method is one of the most promising techniques for obtaining a better calibration of the Cepheid period-luminosity relation by means of interferometric measurements of accurate diameters. In this paper we present new wav
Autor:
Tyler E. Nordgren, C. Papaliolios, Dimitar Sasselov, Massimo Marengo, Margarita Karovska, J. T. Armstrong
Publikováno v:
Astrophysics and Space Science. 286:185-190
We present a new method to compute wavelength- and phase-dependent limb darkening corrections for classical Cepheids. These corrections are derived from hydrodynamic simulations and radiative transfer modeling with a full set of atomic and molecular
Autor:
Tyler E. Nordgren, H. M. Dyck
Publikováno v:
The Astronomical Journal. 124:541-545
We review the systematic variation between optical- and infrared-wavelength angular diameters reported for stars in the approximate range of spectral types K0–M6. We show that there is a correlation between the ratio of angular diameters and the de
Publikováno v:
The Astronomical Journal. 123:3380-3386
Direct diameter observations of Cepheid variables are used to calibrate the Barnes-Evans Cepheid surface brightness relation. Fifty-nine separate Cepheid diameter measurements from four different optical interferometers are used to calculate surface
Publikováno v:
The Astronomical Journal. 122:2707-2712
The Navy Prototype Optical Interferometer (NPOI) has been used to measure the angular diameters of 41 late-type giant and supergiant stars previously observed with the Mark III optical interferometer. Sixteen of these stars have published angular dia
Autor:
David Mozurkewich, Arsen R. Hajian, Andrew F. Boden, Christian A. Hummel, Tyler E. Nordgren, N. Ginestet, J.-M. Carquillat, R. F. Griffin
Publikováno v:
The Astronomical Journal. 121:1623-1635
We present a three-dimensional solution for the orbit of the double star Omicron Leonis, based on new photoelectric radial velocity data mainly from the Observatoire de Haute-Provence and on interferometric data obtained with the Navy Prototype Optic
Publikováno v:
The Astrophysical Journal. 544:176-187
Using complete redshift catalogs, we have compiled a list of galaxy pairs based solely on a pairs pro- jected separation, and velocity diUerence, *V. We have made high-velocity precision H I observations r p , of each galaxy in the sample and have re
Autor:
Robert B. Hindsley, J. T. Armstrong, Jeffrey J. Sudol, Tyler E. Nordgren, Arsen R. Hajian, C. A. Hummel, M. E. Germain
Publikováno v:
The Astrophysical Journal. 543:972-978
We present mean angular diameters for two cepheid variables, alpha Ursae Minoris and zeta Geminorum, determined with the Navy Prototype Optical Interferometer (NPOI). We present linear radii for these cepheids and two additional cepheids, delta Cephe