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Resolving the 3D structure of RS Oph, the fastest repeater among symbiotic recurrent-novae

Submitted by evlbi_beheer on Mon, 12/05/2022 - 11:38

by Ulisse Munari (INAF Padova, Italy), Marcello Giroletti (INAF Bologna, Italy), Benito Marcote (JIVE, the Netherlands), Tim J. O’Brien (Jodrell Bank, UK), Péter Veres (CSPAR, USA), Jun Yang (Chalmers Univ. Onsala, Sweden), David R. A. Williams (Jodrell Bank, UK), and Patrick Woudt (Univ. Cape Town, RSA)

Radio-loud Quasars above Redshift 4: VLBI Imaging of an Extended Sample

Submitted by evlbi_beheer on Thu, 08/18/2022 - 16:03


by Máté Krezinger (ELTE, Hungary), Krisztina Perger (CSFK, Hungary), Krisztina É. Gabányi (ELTE, Hungary), Sándor Frey (CSFK, Hungary), Leonid I. Gurvits (JIVE, the Netherlands), Zsolt Paragi (JIVE, the Netherlands), Tao An (SHAO, China), Yingkang Zhang (SHAO, China), Hongmin Cao (SHNU, China), Tullia Sbarrato (INAF, Italy)

EVN/JIVE Newsletter - Edition 63 September 2022

Submitted by evlbi_beheer on Thu, 08/18/2022 - 15:16

Welcome to the September 2022 issue of the EVN/JIVE Newsletter.

A lot has happened since May. Most important we have finally been able to attend meetings in person and share the lively and collaborative spirit our VLBI community has always shared. The 15th EVN Symposium in Cork and the VLBI Special session at the IAU GA in Busan are important landmarks for a return to normality.

News from ORP

Submitted by evlbi_beheer on Thu, 08/18/2022 - 14:27


by ORP Executive Management Team
 

OPTICON RadioNet Pilot (ORP) is one of the European Commission's 'pilot' programs under EC H2020, launched in March 2021. This four-year project brings together 37 institutions to support and develop seamless access to radio and optical facilities. Through various processes, ORP brings together radio and optical astronomers to create a stronger community to better exploit the opportunities of multi-wavelength science and to benefit from each other's expertise.

Radio properties of the OH megamaser galaxy IIZw 096

Submitted by evlbi_beheer on Thu, 08/18/2022 - 13:31


by Wu Hong (Guizhou Univeristy), Wu Zhongzu(Guizhou University), Sotnikova Yu (SAO, Russia), Chen Yongjun (SHAO China), Zhang Bo (SHAO China), Mufakharov T(SAO, Russia), Shen Zhiqiang (SHAO, China), Chen Xi (Guangzhou University, China), Mikhailov A (SAO Russia), Mingaliev M (SAO Russia), Han Xianming L, Misra Prabhakar