Zobrazeno 1 - 10
of 31
pro vyhledávání: '"B. D. Savage"'
Autor:
Katherine C. Roth, David J. Sahnow, J. C. Howk, George Sonneborn, B. D. Savage, D. G. York, Alfred Vidal-Madjar, Scott D. Friedman, Erik Wilkinson, Thomas B. Ake, K. R. Sembach, B-G Andersson
Publikováno v:
The Astrophysical Journal. 538:L39-L42
Autor:
H. W. Moos, W. C. Cash, L. L. Cowie, A. F. Davidsen, A. K. Dupree, P. D. Feldman, S. D. Friedman, J. C. Green, R. F. Green, C. Gry, J. B. Hutchings, E. B. Jenkins, J. L. Linsky, R. F. Malina, A. G. Michalitsianos, B. D. Savage, J. M. Shull, O. H. W. Siegmund, T. P. Snow, G. Sonneborn, A. Vidal-Madjar, A. J. Willis, B. E. Woodgate, D. G. York, T. B. Ake, B-G Andersson, J. P. Andrews, R. H. Barkhouser, L. Bianchi, W. P. Blair, K. R. Brownsberger, A. N. Cha, P. Chayer, S. J. Conard, A. W. Fullerton, G. A. Gaines, R. Grange, M. A. Gummin, G. Hebrard, G. A. Kriss, J. W. Kruk, D. Mark, D. K. McCarthy, C. L. Morbey, R. Murowinski, E. M. Murphy, W. R. Oegerle, R. G. Ohl, C. Oliveira, S. N. Osterman, D. J. Sahnow, M. Saisse, K. R. Sembach, H. A. Weaver, B. Y. Welsh, E. Wilkinson, W. Zheng
Publikováno v:
The Astrophysical Journal. 538:L1-L6
The Far Ultraviolet Spectroscopic Explorer satellite observes light in the far-ultraviolet spectral region, 905 - 1187 A with high spectral resolution. The instrument consists of four coaligned prime-focus telescopes and Rowland spectrographs with mi
Autor:
B. D. SAVAGE
Publikováno v:
The ANNALS of the American Academy of Political and Social Science. 568:235-249
Publikováno v:
The Astrophysical Journal. 661:1347-1347
Publikováno v:
The Astrophysical Journal. 404:124
An analysis of observations of 24 absorption lines produced near zero redshift by Milky Way disk and halo gas along the sight line to 3C 273 is presented. The reduced spectra have a resolution of about 20 km/s (FWHM) with broad wings and an SNR of 13
Autor:
Nolan R. Walborn, You-Hua Chu, J. V. Feitzinger, Th. Schmidt-Kaler, B. D. Savage, W. Seggewiss
Publikováno v:
Symposium - International Astronomical Union. 108:263-270
Autor:
B. D. Savage, A. D. Code
Publikováno v:
Symposium - International Astronomical Union. 36:302-314
The equivalent width of the blended line at Lyman α is given for 48 stars measured with the OAO-A2 scanning spectrometer. This provides an upper limit to the neutral hydrogen column density. In the Orion association these upper limits are significan
Autor:
R. E. Danielson, B. D. Savage
Publikováno v:
Symposium - International Astronomical Union. 35:112-125
It appears that it is necessary to look for oscillatory (i.e. overstable) instabilities as the cause of energy transport in sunspots. Making use of recent calculations on the hydromagnetic stability of thermally unstable layers with open boundary con
Autor:
R. C. Bless, B. D. Savage
Publikováno v:
Symposium - International Astronomical Union. 36:28-35
We present a preliminary analysis of a number of spectrophotometric scans of reddened and unreddened early-type stars obtained with the OAO-A2 satellite. The principal findings are: (1) all the extinction curves show a ‘bump’ at 1/λ ≈ 4.5; (2)
Autor:
A. D. Code, B. D. Savage
Publikováno v:
Transactions of the International Astronomical Union. 15:685-695