Optical interferometry of early-type stars with PAVO@ CHARA–I. Fundamental stellar properties
We present interferometric observations of seven main-sequence and three giant stars with
spectral types from B2 to F6 using the Precision Astronomical Visible Observations beam …
spectral types from B2 to F6 using the Precision Astronomical Visible Observations beam …
VISION: A six-telescope fiber-fed visible light beam combiner for the navy precision optical interferometer
EV Garcia, MW Muterspaugh, G van Belle… - Publications of the …, 2016 - iopscience.iop.org
Visible-light long baseline interferometry holds the promise of advancing a number of
important applications in fundamental astronomy, including the direct measurement of the …
important applications in fundamental astronomy, including the direct measurement of the …
Angular sizes, radii, and effective temperatures of b-type stars from optical interferometry with the chara array
We present interferometric observations of 25 spectral type-B stars that were made with the
Precision Astronomical Visible Observations and the CLassic Interferometry with Multiple …
Precision Astronomical Visible Observations and the CLassic Interferometry with Multiple …
Angular Sizes and Effective Temperatures of O-type Stars from Optical Interferometry with the CHARA Array
We present interferometric observations of six O-type stars that were made with the
Precision Astronomical Visible Observations beam combiner at the Center for High Angular …
Precision Astronomical Visible Observations beam combiner at the Center for High Angular …
Phase-referenced Interferometry and Narrow-angle Astrometry with SUSI
The Sydney University Stellar Interferometer (SUSI) now incorporates a new beam
combiner, called the Microarc-second University of Sydney Companion Astrometry …
combiner, called the Microarc-second University of Sydney Companion Astrometry …
Recent technical and scientific highlights from the CHARA Array
HA McAlister, TA Ten Brummelaar… - Optical and Infrared …, 2012 - spiedigitallibrary.org
The CHARA Array is a six-telescope optical/IR interferometer managed by the Center for
High Angular Resolution Astronomy of Georgia State University and located at Mount Wilson …
High Angular Resolution Astronomy of Georgia State University and located at Mount Wilson …
Fundamental Properties of O and B Stars with Optical Interferometry
We used interferometric observations made with the CHARA Array of 25 B-type stars and 6
O-type stars to obtain precise measurements of angular size, radius, and effective …
O-type stars to obtain precise measurements of angular size, radius, and effective …
[图书][B] Astrophysical Laboratories and Advanced Imaging Techniques for Testing Stellar Models: Eclipsing Binaries, High Contrast Imaging, and Optical Interferometry
EV Garcia - 2016 - search.proquest.com
Astrophysical Laboratories and Advanced Imaging Techniques for Testing Stellar Models:
Eclipsing Binaries, High Contrast Imaging Page 1 Astrophysical Laboratories and Advanced …
Eclipsing Binaries, High Contrast Imaging Page 1 Astrophysical Laboratories and Advanced …
Alternative approach to precision narrow-angle astrometry for Antarctic long baseline interferometry
The conventional approach to high-precision narrow-angle astrometry using a long baseline
interferometer is to directly measure the fringe packet separation of a target and a nearby …
interferometer is to directly measure the fringe packet separation of a target and a nearby …
[引用][C] Alternative approach to precision narrow-angle astrometry for Antarctic long baseline interferometry
AC Rizzuto, PG Tuthill, JG Robertson… - 2014 - SPIE-The International Society for …