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P. I. Pápics

7 papers here

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

author position
  • middle author7

Across the 7 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR7
ORCID 0000-0002-3697-1664
same name
  • P. I. Pápics — 1 paper

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
20092016
most citedKepler's first view of O-star variability: K2 data of five O stars in Campaign 0 as a proof-of-concept for O-star asteroseismology

46 citations · 154 across the 7 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.SR2016★ 34 cited

Vetting Galactic Leavitt Law Calibrators using Radial Velocities: On the Variability, Binarity, and Possible Parallax Error of 19 Long-period Cepheids

R. I. Anderson, S. Casertano, A. G. Riess +9

We investigate the radial velocity (RV) variability and spectroscopic binarity of 19 Galactic long-period (Ppuls​≳10 d) classical Cepheid variable stars whose trig…

astro-ph.SR2016★ 18 cited

G 207-9 and LP 133-144: light curve analysis and asteroseismology of two ZZ Ceti stars

Zs. Bognár, M. Paparó, L. Molnár +4

G 207-9 and LP 133-144 are two rarely observed ZZ Ceti stars located in the middle and close to the blue edge of the ZZ Ceti instability domain, respectively. We aimed to observe t…

astro-ph.SR2016★ 31 cited

Stellar modelling of Spica, a high-mass spectroscopic binary with a beta Cep variable primary component

A. Tkachenko, J. M. Matthews, C. Aerts +16

Binary stars provide a valuable test of stellar structure and evolution, because the masses of the individual stellar components can be derived with high accuracy and in a model-in…

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