Investigation of submillimeter astronomical site potential of Ding-Ri, Tibet
1996; Elsevier BV; Volume: 20; Issue: 2 Linguagem: Inglês
10.1016/0275-1062(96)82061-3
ISSN1879-128X
Tópico(s)Astronomy and Astrophysical Research
ResumoThe existence of a luminous bridge between the quasar Markarian 205 and the galaxy NGC 4319 has long been known as evidence that quasars are not at their redshift distance. Special X-ray observations were made which supported this particular evidence but the observations were not reported. Those observations are now recovered from the Einstein Laboratory Archives. It is shown how a very small allocation of observing time from the new X-ray telescope ROSAT could further resolve this crucial question in extragalactic astronomy.
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