MPIfR: Der MeerKAT-Absorptionslinienatlas – Raumfahrer.net

MPIfR: Zehn neue Neutronensterne für Terzan 5 - Raumfahrer.net

Entdeckung und Untersuchung mehrerer seltener und ungewöhnlicher Pulsare in einem dichten Sternhaufen mit Hilfe von MeerKAT/Südafrika und dem Green-Bank-Teleskop/USA. Eine Pressemeldung des Max-Planck-Instituts für Radioastronomie, Bonn. Quelle: Max-Planck-Institut für Radioastronomie 16. Juli 2024. 16. Juli 2024 – Ein internationales Team unter der Leitung von Forschenden des Max-Planck-Instituts für Gravitationsphysik, des Max-Planck-Instituts für Radioastronomie und des […]

MeerKAT+: the MeerKAT Extension

Leichtestes Schwarzes Loch oder schwerster Neutronenstern? – Raumfahrer.net

MPI for Gravitational Physics (@[email protected])

Attached: 1 image Lightest black hole or heaviest neutron star? MeerKAT uncovers a mysterious object at the boundary between black holes and neutron stars 🆕➡️ https://www.aei.mpg.de/1112157/lightest-black-hole-or-heaviest-neutron-star “When we looked at Hubble images of NGC 1851, we saw nothing at that position.” (Prajwal Voraganti Padmanabh, postdoc at @mpi_grav Hannover) Pic: @MPIfR_Bonn; Daniëlle Futselaar (artsource.nl) #MeerKAT #TRAPUM #Pulsar #BlackHole #Astrophysics #Astronomy

Trapani, in chiusura il nuovo attaccante. Siracusa più vicino a Sarao

In chiusura la trattativa tra il Trapani e Convitto. Super offerta alla Vibonese e al giocatore. Lasciato Sarao su cui è forte il Siracusa

The SARAO MeerKAT 1.3 GHz Galactic Plane Survey

We present the SARAO MeerKAT Galactic Plane Survey (SMGPS), a 1.3 GHz continuum survey of almost half of the Galactic Plane (251°$\le l \le$ 358°and 2°$\le l \le$ 61°at $|b| \le 1.5°$). SMGPS is the largest, most sensitive and highest angular resolution 1 GHz survey of the Plane yet carried out, with an angular resolution of 8" and a broadband RMS sensitivity of $\sim$10--20 $μ$ Jy/beam. Here we describe the first publicly available data release from SMGPS which comprises data cubes of frequency-resolved images over 908--1656 MHz, power law fits to the images, and broadband zeroth moment integrated intensity images. A thorough assessment of the data quality and guidance for future usage of the data products are given. Finally, we discuss the tremendous potential of SMGPS by showcasing highlights of the Galactic and extragalactic science that it permits. These highlights include the discovery of a new population of non-thermal radio filaments; identification of new candidate supernova remnants, pulsar wind nebulae and planetary nebulae; improved radio/mid-IR classification of rare Luminous Blue Variables and discovery of associated extended radio nebulae; new radio stars identified by Bayesian cross-matching techniques; the realisation that many of the largest radio-quiet WISE HII region candidates are not true HII regions; and a large sample of previously undiscovered background HI galaxies in the Zone of Avoidance.