B 1849 + 00 probes the tiny - scale molecular gas ?
نویسندگان
چکیده
In this paper we present and discuss the great difference in OH absorption spectra against PSR B1849+00 and SNR G33.6+0.1 along the same line-ofsight. This finding is important as it clearly demonstrates that statistics of absorbing molecular gas depends on the size of the background source.
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تاریخ انتشار 2003