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F. Barblan

Identifiers

  • name variant F. Barblan 0.60 · backfill

Papers (16)

  1. Gaia Data Release 2: Observational Hertzsprung-Russell diagrams astro-ph.SR · 2018 · author #146
  2. Gaia Data Release 2: Summary of the variability processing & analysis results astro-ph.SR · 2018 · author #29
  3. Close binary evolution. III. Impact of tides, wind magnetic braking, and internal angular momentum transport astro-ph.SR · 2017 · author #10
  4. Gaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae stars astro-ph.SR · 2017 · author #153
  5. Gaia eclipsing binary and multiple systems. Two-Gaussian models applied to OGLE-III eclipsing binary light curves in the Large Magellanic Cloud astro-ph.IM · 2017 · author #5
  6. Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects astro-ph.SR · 2017 · author #145
  7. Gaia eclipsing binary and multiple systems. Supervised classification and self-organizing maps astro-ph.IM · 2017 · author #2
  8. Gaia Data Release 1: The variability processing & analysis and its application to the south ecliptic pole region astro-ph.IM · 2017 · author #42
  9. Stellar variability in open clusters. II. Discovery of a new period-luminosity relation in a class of fast-rotating pulsating stars in NGC 3766 astro-ph.SR · 2016 · author #5
  10. Physics of massive stars relevant for the modeling of Wolf-Rayet populations astro-ph.SR · 2016 · author #6
  11. On the interpretation of new late B- and early A-type periodic variable stars in NGC 3766 astro-ph.SR · 2013 · author #3
  12. Stellar variability in open clusters. I. A new class of variable stars in NGC 3766 astro-ph.SR · 2013 · author #2
  13. The Gaia mission astro-ph.IM · 2013 · author #6
  14. The impact of Gaia and LSST on binary stars and exo-planets astro-ph.IM · 2012 · author #6
  15. VLT multi-object spectroscopy of 33 eclipsing binaries in the Small Magellanic Cloud. New distance and depth of the SMC, and a record-breaking apsidal motion astro-ph.SR · 2010 · author #3
  16. Evolution towards the critical limit and the origin of Be stars astro-ph · 2007 · author #4

Mentions

  • 1310.6488 #3 · backfill · confidence 0.70 F. Barblan
  • 1304.5266 #2 · backfill · confidence 0.70 F. Barblan
  • 1303.0303 #6 · backfill · confidence 0.70 F. Barblan
  • 1201.5140 #6 · backfill · confidence 0.70 F. Barblan
  • 1005.4336 #3 · backfill · confidence 0.70 F. Barblan
  • 0711.1735 #4 · backfill · confidence 0.70 F. Barblan

Frequent Coauthors