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T. Saguner

3 papers hereh-index 364 citations11 works total

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

author position
  • first author1
  • last author1

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

fields
  • astro-ph.GA2
  • astro-ph.SR1

identity via Semantic Scholar / OpenAlex

most citedProperties, evolution and morpho-kinematical modelling of the very fast nova V2672 Oph (Nova Oph 2009), a clone of U Sco

55 citations · 62 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2011

First Results for the Solar Neighborhood of the Asiago Red Clump Survey

M. Valentini, U. Munari, T. Saguner +4

The Asiago Red Clump Spectroscopic Survey (ARCS) is an ongoing survey that provides atmospheric parameters, distances and space velocities of a well selected sample of Red Clump st…

astro-ph.GA2010★ 7 cited

A spectroscopic survey of faint, high-galactic latitude red clump stars. II. The medium resolution sample

T. Saguner, U. Munari, M. Fiorucci +1

Aims. The goal of our survey is to provide accurate and multi-epoch radial velocities, atmospheric parameters (Teff, log g and [M/H]), distances and space velocities of faint Red C…

astro-ph.SR2010★ 55 cited

Properties, evolution and morpho-kinematical modelling of the very fast nova V2672 Oph (Nova Oph 2009), a clone of U Sco

U. Munari, V. A. R. M. Ribeiro, M. F. Bode +1

V2672 Oph reached maximum brightness V=11.35 on 2009 August 16.5. With observed t2(V)=2.3 and t3(V)=4.2 days decline times, it is one of the fastest known novae, being rivalled onl…

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