Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Richard H. Buss"'
Autor:
Bhaswar Sen, Daniel Cumpton, Michael G. Grotenhuis, Glen Jaross, Wei Yu, Jian Zeng, Richard H. Buss, Jianguo Niu, Wen-Hao Li, Haifeng Qian, M. K. Rama Varma Raja, Maria Caponi, Trevor Beck, Xiangqian Wu, Lawrence E. Flynn, Scott J. Janz, Quanhua Liu, William Johnsen, Derek Stuhmer, Chunhui Pan, Eric Beach, Cristina Owen
Publikováno v:
Journal of Geophysical Research: Atmospheres. 119:6170-6180
This paper evaluates the first 15 months of the Ozone Mapping and Profiler Suite (OMPS) Sensor Data Record (SDR) acquired by the nadir sensors and processed by the National Oceanic and Atmospheric Administration Interface Data Processing Segment. The
Autor:
Ji-Cheng Liu, Thomas M. Brown, Jeffrey W. Kruk, Richard H. Buss, Stephan R. McCandliss, M. Marsha Allen
Publikováno v:
The Astrophysical Journal. 430:630
From far-ultraviolet (FUV) spectra of B stars taken with the Hopkins Ultraviolet Telescope (HUT) and Voyager space observations, we determine the far-ultraviolet extinction by Galactic dust and hydrogen absorption in the local spiral-arm clouds towar
Autor:
Arthur F. Davidsen, Paul D. Feldman, William P. Blair, Stephan R. McCandliss, Jeffrey W. Kruk, Charles W. Bowers, Richard H. Buss
Publikováno v:
The Astrophysical Journal. 416:372
A unique flux-calibrated spectrum, extending to the Lyman limit of the Wolf-Rayet star EZ CMa (also known as WR 6, HD 50896, spectral type WN5) has been recorded by the Hopkins Ultraviolet Telescope. We compare the spectrum to a pure He continuum mod
Publikováno v:
The Astrophysical Journal. 372:281
The mid-infrared spectra of carbon giant stars with hot companions are investigated in order to search for infrared emission bands from polycyclic aromatic hydrocarbons (PAH) in the envelopes of the C giants. A strong 8-micron emission band found in
Publikováno v:
The Astrophysical Journal. 347:977
The circumstellar grains of two hot evolved postasymptotic giant branch stars, HD 89353 and HD 213985, are examined, deriving the extinction around 2175 A. An unsuccessful attempt to detect 6614 A diffuse band absorption arising from the grains impli
Publikováno v:
The Astrophysical Journal. 321:921
The UV extinction and element depletions in the circumstellar envelope Alpha Sco are investigated using IUE, Copernicus, and AS data of Alpha Sco B which can be seen in absorption through the cool-star envelope. The circumstellar reddening, depletion
Autor:
Richard H. Buss, Theodore P. Snow
Publikováno v:
The Astrophysical Journal. 335:331
Ultraviolet and infrared spectra were obtained in order to study grains in cool star and hot star syncretic type binaries. Grains are found in only about half of the syncretic systems. The results suggest that grains have not formed in many syncretic