Characteristics of the distribution of proton flares on the solar surface
1995; Elsevier BV; Volume: 19; Issue: 1 Linguagem: Inglês
10.1016/0275-1062(95)90028-4
ISSN1879-128X
Tópico(s)Stellar, planetary, and galactic studies
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.
Referência(s)