output
20022026
most citedObservations of the Crab Nebula with H.E.S.S

863 citations

Showing 2020Show all

36 papers · 1 filter

astro-ph.SR202010 cited

A Multi-Epoch Study of Radio Continuum Emission from MassiveProtostars

W. O. Obonyo, S. L. Lumsden, M. G. Hoare +2

We report the results of the Jansky Very Large Array (JVLA) observation of five massive protostars at 6 and 22.2 GHz. The aim of the study was to compare their current fluxes and p…

astro-ph.EP202067 cited

Size and structures of disks around very low mass stars in the Taurus star-forming region

Nicolas T. Kurtovic, Paola Pinilla, Feng Long +7

We aim to estimate if structures, such as cavities, rings, and gaps, are common in disks around VLMS and to test models of structure formation in these disks. We also aim to compar…

astro-ph.SR202049 cited

Wind-envelope interaction as the origin of the slow cyclic brightness variations of luminous blue variables

Luca Grassitelli, Norbert Langer, Jonathan Mackey +4

Luminous blue variables (LBVs) are hot, very luminous massive stars displaying large quasi-periodic variations in brightness, radius,and photospheric temperature, on timescales of…

astro-ph.HE202029 cited

Systematic Study of Acceleration Efficiency in Young Supernova Remnants with Nonthermal X-ray Observations

Naomi Tsuji, Yasunobu Uchiyama, Dmitry Khangulyan +1

Cutoff energy in a synchrotron radiation spectrum of a supernova remnant (SNR) contains a key parameter of ongoing particle acceleration. We systematically analyze 11 young SNRs, i…

cond-mat.mes-hall202022 cited

Probing non-Hermitian phase transitions in curved space via quench dynamics

Ygor Pará, Giandomenico Palumbo, Tommaso Macrì

Non-Hermitian Hamiltonians are relevant to describe the features of a broad class of physical phenomena, ranging from photonics and atomic and molecular systems to nuclear physics…

astro-ph.SR202013 cited

LOFAR observations of radio burst source sizes and scattering in the solar corona

Pearse C. Murphy, Eoin P. Carley, Aoife Maria Ryan +2

Low frequency radio wave scattering and refraction can have a dramatic effect on the observed size and position of radio sources in the solar corona. The scattering and refraction…