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A. Spang

44 papers hereh-index 211.9k citations98 works total

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

author position
  • middle author33
  • last author4

Across the 37 of 44 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR24
  • astro-ph.IM9
  • astro-ph7
  • astro-ph.EP3
  • physics.optics1
same name
  • A. Spang — 7 papers, h 4
  • A. Spang — 6 papers
  • A. Spang — 2 papers, h 2
  • A. Spang — 1 paper, h 38
  • A. Spang — 1 paper, h 49

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
20062023
most citedRadiative hydrodynamics simulations of red supergiant stars. III. Spectro-photocentric variability, photometric variability, and consequences on Gaia measurements

114 citations · 1k across the 44 of their papers we have counts for

collaborators
Showing 2011Show all

3 papers · 1 filter

astro-ph.SR2011★ 15 cited

Chromosphere of K giant stars Geometrical extent and spatial structure detection

P. Berio, T. Merle, F. Thevenin +19

We aim to constrain the geometrical extent of the chromosphere of non-binary K giant stars and detect any spatial structures in the chromosphere. We performed observations with the…

astro-ph.SR2011★ 46 cited

The 2011 outburst of the recurrent novaT Pyx. Evidence for a face-on bipolar ejection

Olivier Chesneau, A. Meilland, D. P. K. Banerjee +19

We report on near-IR interferometric observations of the outburst of the recurrent nova T Pyx. We obtained near-IR observations of T Pyx at dates ranging from t=2.37d to t=48.2d af…

astro-ph.SR2011★ 46 cited

The galactic unclassified B[e] star HD 50138. II. Interferometric constraints on the close circumstellar environment

Marcelo Borges Fernandes, Anthony Meilland, Philippe Bendjoya +7

HD 50138 is a southern star that presents the B[e] phenomenon, but its evolutionary stage is still not well known. This object presents spectral variability, which can be explained…

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