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A. Parmar

4 papers hereh-index 71k citations23 works total

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • A. Parmar — 103 papers, h 44
  • A. Parmar — 20 papers, h 4
  • A. Parmar — 12 papers, h 5
  • A. Parmar — 9 papers, h 2
  • A. Parmar — 8 papers
  • A. Parmar — 5 papers, h 3

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

most citedBeppoSAX spectroscopy of the luminous X-ray sources in M33

22 citations · 22 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph2001★ 22 cited

BeppoSAX spectroscopy of the luminous X-ray sources in M33

A. N. Parmar, L. Sidoli, T. Oosterbroek +6

The nearby galaxy M33 was observed by the imaging X-ray instruments on-board BeppoSAX. Two observations at different phases of the 105.9 day intensity cycle of the luminous central…

astro-ph2000

Comptonization in X-ray bright neutron star globular cluster systems

M. Guainazzi, A. N. Parmar, T. Oosterbroek

A BeppoSAX survey of bright Neutron Star (NS) systems in globular clusters, together with the results obtained on Galactic LMXRB, suggests that a two-component model is a reasonabl…

astro-ph2000

Cyclotron lines in X-ray pulsars as a probe of relativistic plasmas in superstrong magnetic fields

D. Dal Fiume, Filippo Frontera, Nicola Masetti +7

The systematic search for the presence of cyclotron lines in the spectra of accreting X-ray pulsars is being carried on with the BeppoSAX satellite since the beginning of the missi…

astro-ph2000

BeppoSAX spectrum of GRB971214: evidence of a substantial energy output during afterglow

D. Dal Fiume, L. Amati, L. A. Antonelli +18

We report the X/gamma-ray spectrum of GRB971214 and of its afterglow. The afterglow was measured few hours after the main event and for an elapsed time of more than two days. The m…

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