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20052025
most citedLow-Frequency Radio Absorption in Cassiopeia A

46 citations · 473 across the 27 of their papers we have counts for

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Showing 2018Show all

5 papers · 1 filter

astro-ph.HE2018★ 17 cited

A low-frequency view of mixed-morphology supernova remnant VRO 42.05.01, and its neighbourhood

M. Arias, J. Vink, M. Iacobelli +7

Mixed-morphology supernova remnants (MM SNRs) are a mysterious class of objects that display thermal X-ray emission within their radio shell. They are an older class of SNRs, and a…

astro-ph.HE2018★ 24 cited

Molecular gas toward supernova remnant Cassiopeia A

Ping Zhou, Jiang-Tao Li, Zhi-Yu Zhang +5

We mapped 12CO J=1-0, 12CO J=2-1, 13CO J=1-0, and 13CO J=2-1 lines toward supernova remnant (SNR) Cassiopeia A with the IRAM 30m telescope. The molecular clouds (MCs) along the lin…

astro-ph.SR2018★ 19 cited

On the evolutionary state of massive stars in transition phases in M33

M. Kourniotis, M. Kraus, M. L. Arias +2

The advanced stages of several high-mass stars are characterized by episodic mass loss shed during phases of instability. Key for assigning these stars a proper evolutionary state…

astro-ph.SR2018★ 41 cited

Resolving the kinematics of the disks around Galactic B[e] supergiants

Grigoris Maravelias, Michaela Kraus, Lydia S. Cidale +4

B[e] Supergiants are luminous evolved massive stars. The mass-loss during this phase creates a complex circumstellar environment with atomic, molecular, and dusty regions usually f…

astro-ph.HE2018★ 46 cited

Low-Frequency Radio Absorption in Cassiopeia A

M. Arias, J. Vink, F. de Gasperin +3

Cassiopeia A is one of the best-studied supernova remnants. Its shocked ejecta emits brightly in radio and X-rays. Its unshocked ejecta can be studied through infrared emission, th…