489 citations
- Netherlands Institute for Radio AstronomyNL18 papers
- Thüringer Landessternwarte TautenburgDE11 papers
- Leibniz Institute for Astrophysics PotsdamDE9 papers
- Leiden UniversityNL9 papers
- Radboud University NijmegenNL9 papers
- Bielefeld UniversityDE8 papers
- Rutherford Appleton LaboratoryGB8 papers
- University of GroningenNL8 papers
- University of ManchesterGB8 papers
- Astronomy and SpaceAU7 papers
- Centre National de la Recherche ScientifiqueFR7 papers
- Commonwealth Scientific and Industrial Research OrganisationAU7 papers
86 papers
RAD@home discovery of a bow-and-arrow radio galaxy tracing a ~560 kpc bow-shock structure in a multi-halo environment
Ananda Hota, Pratik Dabhade, Shubhrangshu Ghosh +9
We report the RAD@home citizen science discovery of a unique bow-and-arrow-shaped radio galaxy (BAARG; RAD J104501.6+352852, z = 0.159) identified in LoTSS DR2. The source exhibits…
The LOFAR Two-metre Sky Survey: VII. Third Data Release
T. W. Shimwell, M. J. Hardcastle, C. Tasse +99
We present the third data release of the LOFAR Two-metre Sky Survey (LoTSS-DR3). The survey images cover 88% of the northern sky and were created from 12,950 hrs of data (18.6 PB)…
Is the nitrogen-rich source PN K4-47 a true planetary nebula?
Thomas Steinmetz, Tomasz Kaminski, David Jones +3
PN K4-47 is a young planetary nebula that exhibits shock-excited bipolar lobes and a complex molecular environment, with the highest number of molecules detected within a planetary…
Gauge gravitation theory in Riemann-Cartan space-time and the nonsingular Universe
A. V. Minkevich
The gauge gravitation theory in the Riemann-Cartan space-time is investigated in order to solve the fundamental problems of the general relativity theory. The constraints for indef…
Magnetic fields in planetary nebulae detected through non-thermal radio continuum emission
Marcin Hajduk, Timothy Shimwell, Glenn White +3
Context. Planetary nebulae are shells ejected by low- and intermediate-mass stars. The slow wind ejected by the asymptotic giant branch star is compressed by a fast stellar wind to…
Source location and evolution of a multi-lane type II radio burst
P. Zucca, P. Zhang, K. Kozarev +8
Shocks in the solar corona can accelerate electrons that in turn generate radio emission known as type II radio bursts. The characteristics and morphology of these radio bursts in…