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M. Orio

41 papers hereh-index 17803 citations49 works total

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

author position
  • first author5
  • middle author17
  • last author7

Across the 29 of 41 papers where every author was matched, so the position is known.

fields
  • astro-ph16
  • astro-ph.HE15
  • astro-ph.SR9
  • astro-ph.IM1
same name
  • M. Orio — 70 papers, h 23
  • M. Orio — 7 papers, h 30
  • M. Orio — 2 papers, h 1

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
19962026
most citedThe Extraordinary X-ray Light Curve of the Classical Nova V1494 Aquilae (1999 #2) in Outburst: The Discovery of Pulsations and a "Burst"

69 citations · 544 across the 40 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.HE2026

Early Emergence of SSS emission in RS Oph

J. -U. Ness, J. P. Osborne, M. Orio +3

Early in the 2006 outburst of the recurrent nova RS Oph, Swift detected the onset of the super-soft-source (SSS) phase. An XMM-Newton observation on day 26.1 revealed an unusual so…

astro-ph.SR2026

A very rapidly rotating white dwarf in nova YZ Reticuli

G. J. M. Luna, N. Rawat, R. Angeloni +4

YZ Ret (Nova Reticuli 2020) is the first VY Scl-type nova-like variable observed to undergo a classical nova eruption. Following the outburst, timing analysis of 20-s cadence TESS…

astro-ph.HE2026

The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review

Marina Orio, Gerardo Juan M. Luna, Ehud Behar +4

In the 2021 outburst of RS Ophiuchi, the gamma- and the X-ray flux were measured quasi-simultaneously from day 1 after the optical peak, offering the first comprehensive view of sh…

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