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R. J. Glinski P. D. Michaels C. M. Anderson T. W. Schmidt R. G. Sharp M. L. Sitko L. S. Bernstein H. Van Winckel 《Astrophysics and Space Science》2009,323(4):337-344
In this paper we discuss our insights into several key problems in the identification of the Red Rectangle Bands (RRBs). We
have combined three independent sets of observations in order to try to define the constraints guiding the bands. We provide
a summary of the general behavior of the bands and review the evidence for a molecular origin of the bands. The extent, composition,
and possible absorption effects of the bands are discussed. Comparison spectra of the strongest band obtained at three different
spectral resolutions suggests that an intrinsic line width of individual rotational lines can be deduced. Spectroscopic models
of several relatively simple molecules were examined in order to investigate where the current data are weak. Suggestions
are made for future studies to enhance our understanding of these enigmatic bands. 相似文献
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Stephen Kuhlmann Harold Spinka Joseph P. Bernstein Kevin A. Beyer Lisa M. Gades Thomas E. Kasprzyk Antonino Miceli Richard A. Spence Richard Talaga 《Experimental Astronomy》2011,29(3):135-144
The physical boundaries of a fully-depleted CCD can lead to distorted field lines and non-uniform response. We study this
response with a beam of X-rays constrained to a width of less than one pixel (15
\upmu\upmum), and a system to map the CCD response as a function of transverse position. 相似文献