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S. Safi-Harb

113 papers hereh-index 395.6k citations305 works total

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

author position
  • sole author1
  • first author7
  • middle author77
  • last author13

Across the 98 of 113 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE78
  • astro-ph16
  • astro-ph.GA10
  • astro-ph.IM6
  • astro-ph.SR2
  • gr-qc1
same name
  • S. Safi-Harb — 5 papers
  • S. Safi-Harb — 2 papers
  • S. Safi-Harb — 2 papers
  • S. Safi-Harb — 2 papers
  • S. Safi-Harb — 1 paper
  • S. Safi-Harb — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20012026
most citedOverview of the Advanced X-ray Imaging Satellite (AXIS)

77 citations · 555 across the 79 of their papers we have counts for

collaborators
Showing 2005Show all

4 papers · 1 filter

astro-ph2005

A Massive Jet Ejection Event from the Microquasar SS 433 Accompanying Rapid X-Ray Variability

T. Kotani, S. A. Trushkin, R. Valiullin +4

Microquasars occasionally exhibit massive jet ejections which are distinct from the continuous or quasi-continuous weak jet ejections. Because those massive jet ejections are rare…

astro-ph2005

The Plerionic Supernova Remnant G21.5-0.9: In and Out

Heather Matheson, Samar Safi-Harb

The absence of a supernova remnant (SNR) shell surrounding the Crab and other plerions (pulsar wind nebulae) has been a mystery for 3 decades. G21.5-0.9 is a particularly intriguin…

astro-ph2005

A Gemini Observation of the Anomalous X-ray Pulsar 1RXS J170849-400910

Samar Safi-Harb, Jennifer West

The anomalous X-ray pulsars (AXPs) represent a growing class of neutron stars discovered at X-ray energies. While the nature of their multi-wavelength emission mechanism is still u…

astro-ph2005

A Multi-Wavelength Study of the Western Lobe of W50 Powered by the Galactic Microquasar SS 433

A. Moldowan, S. Safi-Harb, Y. Fuchs +1

W50 remains the only supernova remnant (SNR) confirmed to harbor a microquasar: the powerful enigmatic source SS 433. Our past study of this fascinating SNR revealed two X-ray lobe…

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