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Publication
Featured researches published by Roger W. Russell.
The Astrophysical Journal | 1978
William J. Forrest; James R. Houck; J. F. Mccarthy; F. C. Gillett; K. M. Merrill; Judith L. Pipher; Richard C. Puetter; Roger W. Russell; B. T. Soifer; S. P. Willner
Airborne and ground-based observations show that OH 26.5 + 0.6 has strong 10-..mu..m and weak 18-..mu..m silicate absorptions superposed on an overall energy distribution much like a blackbody. The flux level, color temperature, and depth of the 10-..mu..m absorption varied during 2 years of observations. A model of the source as a late-type variable star that has ejected an optically thick dust shell is suggested; the mass-loss rate implied is greater than approx. 10/sup -5/ Msub solar year/sup -1/. The fact that significant flux from the source is observed between 4 and 7 ..mu..m is evidence that oxygen-rich dust has significant opacity in that wavelength range. 3 figures, 1 table.
The Astrophysical Journal | 1975
Roger W. Russell; B. T. Soifer; William J. Forrest
Archive | 1977
Richard C. Puetter; Roger W. Russell; Baruch T. Soifer; S. P. Willner
Archive | 1979
Nancy L. Cohen; J. F. Mccarthy; Roger W. Russell; J. R. Stephens
Archive | 1977
Roger W. Russell; Baruch T. Soifer; S. P. Willner
Archive | 1977
Roger W. Russell; Richard C. Puetter; Baruch T. Soifer; S. P. Willner
Publications of the Astronomical Society of the Pacific | 1976
Baruch T. Soifer; Roger W. Russell; K. M. Merrill
Publications of the Astronomical Society of the Pacific | 1976
Baruch T. Soifer; Roger W. Russell; K. M. Merrill
Archive | 1976
S. P. Willner; Roger W. Russell; Baruch T. Soifer
Archive | 1976
William J. Forrest; F. C. Gillett; James R. Houck; J. F. Mccarthy; K. Michael Merrill; Judith L. Pipher; Richard C. Puetter; Roger W. Russell; Baruch T. Soifer; S. P. Willner
