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researcher

D. Wickramasinghe

42 papers hereh-index 365.3k citations320 works total

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

author position
  • first author2
  • middle author20
  • last author18

Across the 40 of 42 papers where every author was matched, so the position is known.

fields
  • astro-ph19
  • astro-ph.SR19
  • astro-ph.HE2
  • astro-ph.CO1
  • physics.gen-ph1
same name
  • D. Wickramasinghe — 2 papers, h 3
  • D. Wickramasinghe — 2 papers, h 1
  • D. Wickramasinghe — 1 paper, h 5

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
19972025
most citedBinary Star Origin of High Field Magnetic White Dwarfs

231 citations · 1.9k across the 41 of their papers we have counts for

collaborators
Showing 2010Show all

4 papers · 1 filter

astro-ph.HE2010★ 160 cited

Study of measured pulsar masses and their possible conclusions

C. M. Zhang, J. Wang, Y. H. Zhao +6

We study the statistics of 61 measured masses of neutron stars (NSs) in binary pulsar systems, including 18 double NS (DNS) systems, 26 radio pulsars (10 in our Galaxy) with white…

astro-ph.SR2010★ 17 cited

A Common Envelope Binary Star Origin of Long Gamma-ray Bursts

Christopher A. Tout, Dayal T. Wickramasinghe, Herbert H. -B. Lau +2

The stellar origin of gamma-ray bursts can be explained by the rapid release of energy in a highly collimated, extremely relativistic jet. This in turn appears to require a rapidly…

astro-ph.SR2010★ 28 cited

Observations of radio pulses from CU Virginis

V. Ravi, G. Hobbs, D. Wickramasinghe +7

The magnetic chemically peculiar star CU Virginis is a unique astrophysical laboratory for stellar magnetospheres and coherent emission processes. It is the only known main sequenc…

astro-ph.SR2010★ 15 cited

Does GD 356 have a Terrestrial Planetary Companion?

Dayal T. Wickramasinghe, Jay Farihi, Christopher A. Tout +2

GD 356 is unique among magnetic white dwarfs because it shows Zeeman-split Balmer lines in pure emission. The lines originate from a region of nearly uniform field strength (delta…

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