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Marina Orio

3 papers here

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

author position
  • first author1
  • middle author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph1
  • astro-ph.IM1
  • astro-ph.SR1
ORCID 0000-0003-1563-9803

identity via Semantic Scholar / OpenAlex

most citedNLTE model atmospheres for the hottest white dwarfs: Spectral analysis of the compact component in nova V4743 Sgr

75 citations · 75 across the 3 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2007★ 88 cited

X-ray Spectroscopy of the 2006 Outburst of RS Oph

Thomas Nelson, Marina Orio, Joseph P. Cassinelli +3

We present the X-ray grating spectra of the recurrent nova RS Ophiuchi during its 2006 outburst, obtained with the XMM-Newton and Chandra observatories. Two weeks after optical max…

astro-ph2006★ 26 cited

Variability and multi-periodic oscillations in the X-ray light curve of the classical nova V4743 Sgr

E. Leibowitz, M. Orio, R. Gonzalez-Riestra +5

The classical nova V4743 Sgr was observed with XMM-Newton for about 10 hours on April 4 2003, 6.5 months after optical maximum. At this time, this nova had become the brightest sup…

astro-ph2004

A New View of the Supersoft X-Ray Source Cal 87 Observed with XMM-Newton

Marina Orio, Ken Ebisawa, John Heise +1

Cal 87 was observed with XMM-Newton in April of 2003. The source shows a rich emission line spectrum, where lines can be identified if they are red-shifted by 700-1200 km/s. These…

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