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researcher

Orly Gnat

3 papers here

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

author position
  • middle author3

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

fields
  • astro-ph.CO1
  • astro-ph.GA1
  • astro-ph.HE1
ORCID 0000-0002-4244-0237

identity via Semantic Scholar / OpenAlex

most citedPTF11kx: A Type-Ia Supernova with a Symbiotic Nova Progenitor

351 citations · 458 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2018★ 31 cited

CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: dependence on redshift, halo mass and radius

S. Roca-Fàbrega, A. Dekel, Y. Faerman +8

We study the components of cool and warm/hot gas in the circumgalactic medium (CGM) of simulated galaxies and address the relative production of OVI by photoionization versus colli…

astro-ph.CO2012★ 351 cited

PTF11kx: A Type-Ia Supernova with a Symbiotic Nova Progenitor

B. Dilday, D. A. Howell, S. B. Cenko +32

There is a consensus that Type-Ia supernovae (SNe Ia) arise from the thermonuclear explosion of white dwarf stars that accrete matter from a binary companion. However, direct obser…

astro-ph.HE2012★ 76 cited

X-ray emission from supernovae in dense circumstellar matter environments: A search for collisionless shocks

E. O. Ofek, D. Fox, S. B. Cenko +21

(Abridged). The optical light curve of some SNe may be powered by the outward diffusion of the energy deposited by the explosion shock in optically thick circumstellar matter (CSM)…

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