activity
19992023
most citedMapping accretion and its variability in the young open cluster NGC 2264: a study based on u-band photometry

149 citations · 2.4k across the 69 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.GA2022★ 15 cited

Spatial and dynamical structure of the NGC 2264 star-forming region

E. Flaccomio, G. Micela, G. Peres +7

The processes that lead from molecular clouds to protostars, stellar associations, and the evolution of both, are active research topics. The target of this study, NGC2264, is a be…

astro-ph.HE2022★ 28 cited

The supernova remnant SN 1006 as a Galactic particle accelerator

Roberta Giuffrida, Marco Miceli, Damiano Caprioli +6

The origin of cosmic rays is a pivotal open issue of high-energy astrophysics. Supernova remnants are strong candidates to be the Galactic factory of cosmic rays, their blast waves…

astro-ph.HE2022★ 10 cited

A spatially resolved study of hard X-ray emission in Kepler's SNR: indications of different regimes of particle acceleration

Vincenzo Sapienza, Marco Miceli, Aya Bamba +6

Synchrotron X-ray emission in young supernova remnants (SNRs) is a powerful diagnostic tool to study the population of high energy electrons accelerated at the shock front and the…

astro-ph.HE2022★ 25 cited

Additional evidence for a pulsar wind nebula in the heart of SN 1987A from multi-epoch X-ray data and MHD modeling

Emanuele Greco, Marco Miceli, Salvatore Orlando +9

Since the day of its explosion, supernova (SN) 1987A has been closely monitored to study its evolution and to detect its central compact relic. In fact, the formation of a neutron…

astro-ph.HE2022★ 50 cited

Evidence for past interaction with an asymmetric circumstellar shell in the young SNR Cassiopeia A

S. Orlando, A. Wongwathanarat, H. -T. Janka +8

Observations of the SNR Cassiopeia A (Cas A) show asymmetries in the reverse shock that cannot be explained by models describing a remnant expanding through a spherically symmetric…

astro-ph.GA2022★ 27 cited

Negative and Positive Feedback from a Supernova Remnant with SHREC: A detailed Study of the Shocked Gas in IC443

G. Cosentino, I. Jiménez-Serra, J. C. Tan +20

Supernova remnants (SNRs) contribute to regulate the star formation efficiency and evolution of galaxies. As they expand into the interstellar medium (ISM), they transfer vast amou…