Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Miriam M. Nyamai"'
Autor:
Miriam M Nyamai, Justin D Linford, James R Allison, Laura Chomiuk, Patrick A Woudt, Valério A R M Ribeiro, Sumit K Sarbadhicary
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
We present radio observations of the symbiotic recurrent nova V3890 Sagitarii following the 2019 August eruption obtained with the MeerKAT radio telescope at 1.28 GHz and Karl G. Janksy Very Large Array (VLA) at 1.26 to 5 GHz. The radio light curves
Autor:
Iris de Ruiter, Miriam M Nyamai, Antonia Rowlinson, Ralph A M J Wijers, Tim J O’Brien, David R A Williams, Patrick Woudt
We report low-frequency radio observations of the 2021 outburst of the recurrent nova RS Ophiuchi. These observations include the lowest frequency observations of this system to date. Detailed light curves are obtained by MeerKAT at 0.82 and 1.28 GHz
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e76d4a0818d3ddb7bc7889b08f32cef7
http://arxiv.org/abs/2301.10552
http://arxiv.org/abs/2301.10552
Autor:
Laura Chomiuk, Kirill Sokolovsky, Elias Aydi, Ryan Urquhart, Miroslav Filipovic, Jennifer L. Sokoloski, Stuart D. Ryder, Michael Rupen, Koji Mukai, Adam Kawash, Brian D. Metzger, Justin D. Linford, Erik C. Kool, Nirupam Roy, Valério A. R. M. Ribeiro, Amy J. Mioduszewski, Miriam M. Nyamai, Keith W. Bannister, Miriam I. Krauss, T. J. N. Nelson, Jay Strader, Jennifer Weston, T. Finzell
We present radio observations (1--40 GHz) for 36 classical novae, representing data from over five decades compiled from the literature, telescope archives, and our own programs. Our targets display a striking diversity in their optical parameters (e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92795796bcaae8b899b3b87b47c59733
http://arxiv.org/abs/2107.06251
http://arxiv.org/abs/2107.06251
Autor:
Patrick Woudt, V. A. R. M. Ribeiro, Jay Strader, Miriam M. Nyamai, Kirill Sokolovsky, Laura Chomiuk
V445 Puppis is the only helium nova observed to date; its eruption in late 2000 showed high velocities up to 8500 km/s and a remarkable bipolar morphology cinched by an equatorial dust disc. Here we present multi-frequency radio observations of V445
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1da901d96ae2f450f19a0a45fd9882f
Autor:
Pieter Meintjes, Johannes Petrus Marais, A. Odendaal, R. J. Britto, Brian van Soelen, David Murphy, Miriam M Nyamai, Mokhine Motsoaledi, Helene Szegedi, Andry Rajoelimanana, Antonio Martin-Carrillo, John R. Thorstensen, Lorraine Hanlon
Publikováno v:
Scopus-Elsevier
We present optical photometric and spectroscopic observations of three SU UMa-type dwarf novae, i.e. AR Pic, QW Ser and V521 Peg, conducted in 2016 and 2017. These sources were selected from the Catalina Real-Time Transient Survey and observed during