SPECKLE INTERFEROMETRY AT SOAR IN 2010 AND 2011: MEASURES, ORBITS, AND RECTILINEAR FITS
By W. Hartkopf, A. Tokovinin, B. Mason. 2012
258 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/b7c290441506703c493ece540a7c61ca11c5efb1
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In Astronomy and Astrophysics
- A. Tokovinin
- I. Ramírez
- Jorge Meléndez
- B. Mason
- W. Hartkopf
- Debra A. Fischer
- Martin Asplund
- A. Alves-Brito
In Instrumentation
- A. Tokovinin
- I. Ramírez
- B. Mason
- W. Hartkopf
- Jorge Meléndez
- Martin Asplund
- Debra A. Fischer
- T. Pribulla
Citations in the corpus
- Searching for faint companions with VLTI/PIONIER - II. 92 main sequence stars from the Exozodi survey (2014, background): “More recently, the star was resolved as a binary by speckle interferom - try (Hartkopf et al. 2012), showing the presence of a bright companion (∆I = 0.7 mag,∆y = 1.4 mag) at an angular separation of 70.3 mas and a position angle of 60◦.4 (Besselian epoch of observation: 2011.0393 yr).”
- Massive pulsating stars observed by BRITE-Constellation - I. The triple system β Centauri (Agena) (2016, background): “New observations made by means of speckle interferometry (Tokovinin et al. 2010, 2014, 2015; Hartkopf et al. 2012) indicate much smaller and rapidly decreasing separation between the components (Fig.”
- The Solar Twin Planet Search. I. Fundamental parameters of the stellar sample (2014, background): “This object, HIP 67620, is known to have an unresolved (for our spectroscopic observations) faint companion, which is revealed by speckle interferometry (Hartkopf et al. 2012).”
- Speckle Interferometry at SOAR in 2016 and 2017 (2014, background): “This paper continues the series published by Tokovinin, Mason, & Hartkopf (2010a, hereafter TMH10), Tokovinin et al. (2010b), Hartkopf et al. (2012), Tokovinin (2012), Tokovinin et al. (2014), Tokovinin et al. (2015, hereafter SOAR14), and Tokovinin et al. (2016a).”
- RADIAL VELOCITIES OF SOUTHERN VISUAL MULTIPLE STARS (2014, background): “The visual pair AB has a 52-yr eccentric orbit (Hartkopf et al. 2012).”