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Barbara Olmi

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
ORCID 0000-0001-6022-8216

identity via Semantic Scholar / OpenAlex

most citedOn the origin of jet-like features in bow shock pulsar wind nebulae

39 citations · 84 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2019★ 9 cited

Deciphering the Nature of the Pulsar Wind Nebula CTB 87 with XMM-Newton

Benson Guest, Samar Safi-Harb, Austin MacMaster +5

CTB 87 (G74.9+1.2) is an evolved supernova remnant (SNR) which hosts a peculiar pulsar wind nebula (PWN). The X-ray peak is offset from that observed in radio and lies towards the…

astro-ph.HE2019★ 39 cited

On the origin of jet-like features in bow shock pulsar wind nebulae

Barbara Olmi, Niccolò Bucciantini

Bow shock pulsar wind nebulae are a large class of non-thermal synchrotron sources associated to old pulsars, that have emerged from their parent supernova remnant and are directly…

astro-ph.HE2019★ 36 cited

Full-3D relativistic MHD simulations of Bow Shock Pulsar Wind Nebulae: dynamics

Barbara Olmi, Niccolo' Bucciantini

Bow shock pulsar wind nebulae (BSPWNe) are know to show a large variety of shapes and morphologies, both when comparing different objects, and for the same object in different ener…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.