Zobrazeno 1 - 10
of 68
pro vyhledávání: '"Andrew F. Boden"'
Autor:
Guillermo Torres, Gail H. Schaefer, Robert P. Stefanik, David W. Latham, Andrew F. Boden, Narsireddy Anugu, Jeremy W. Jones, Robert Klement, Stefan Kraus, Cyprien Lanthermann, John D. Monnier
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 1, p 31 (2024)
We report long-baseline interferometric observations with the CHARA Array that resolve six previously known double-lined spectroscopic binary systems in the Hyades cluster, with orbital periods ranging from 3 to 358 days: HD 27483, HD 283882, HD 2687
Externí odkaz:
https://doaj.org/article/1cc85ce0070443c4b45d108eeb5363ff
Autor:
Kaspar von Braun, William Bucknew, David R. Ciardi, Ryan S. Buckingham, Zachary Hartman, Andrew F. Boden, Gerald van Belle, Gary Cole, Catherine Clark, Gerard T. van Belle, Genady Pilyavsky
Publikováno v:
The Astrophysical Journal. 922:163
We calculate directly determined values for effective temperature ($T_{\rm EFF}$) and radius ($R$) for 191 giant stars based upon high resolution angular size measurements from optical interferometry at the Palomar Testbed Interferometer. Narrow- to
Autor:
Andrew F. Boden, Rosa M. Torres, Marina Kounkel, Neal J. Evans, Phillip A. B. Galli, Amy J. Mioduszewski, Luis F. Rodríguez, Lee Hartmann, Gisela N. Ortiz-León, John J. Tobin, Sergio A. Dzib, Cesar Briceno, Laurent Loinard
Publikováno v:
Astrophysical Journal, 865(1), 73
We derive the distance and structure of the Perseus molecular cloud by combining trigonometric parallaxes from Very Long Baseline Array (VLBA) observations, taken as part of the GOBELINS survey, and Gaia Data Release 2. Based on our VLBA astrometry,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3765f79c08ddb2cfa5b5f9d247aa1e4c
http://arxiv.org/abs/1808.03499
http://arxiv.org/abs/1808.03499
Autor:
Andrew F. Boden, Phillip A. B. Galli, Juana L. Rivera, Ramachrisna Teixeira, Neal J. Evans, Luis F. Rodríguez, Lee Hartmann, Sergio A. Dzib, John J. Tobin, Amy J. Mioduszewski, Mark H. Heyer, Cesar Briceno, Gisela N. Ortiz-León, Laurent Loinard, Rosa M. Torres, Marina Kounkel
We present new trigonometric parallaxes and proper motions of young stellar objects in the Taurus molecular cloud complex from observations collected with the Very Long Baseline Array as part of the Gould's Belt Distances Survey (GOBELINS). We detect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9823150366a0a8d21e9de90401cdcbd5
http://arxiv.org/abs/1805.09357
http://arxiv.org/abs/1805.09357
Autor:
Luis F. Rodríguez, Laurent Loinard, Juana L. Rivera, John J. Tobin, Amy J. Mioduszewski, Sergio A. Dzib, Neal J. Evans, Andrew F. Boden, D. H. Gudehus, Gerardo Pech, Phillip A. B. Galli, Lee Hartmann, Marina Kounkel, Gisela N. Ortiz-León, Rosa M. Torres, Cesar Briceno, Rosa A. González-Lópezlira
Publikováno v:
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), 834(2), 141
We present the first results of the Gould's Belt Distances Survey (GOBELINS), a project aimed at measuring the proper motion and trigonometric parallax of a large sample of young stars in nearby regions using multi-epoch Very Long Baseline Array (VLB
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::26be6e4dbec084f1280034c815cb58a9
https://resolver.caltech.edu/CaltechAUTHORS:20170111-100932441
https://resolver.caltech.edu/CaltechAUTHORS:20170111-100932441
Autor:
Laurent Loinard, Andrew F. Boden, Sergio A. Dzib, Neal J. Evans, Luis F. Rodríguez, Amy J. Mioduszewski, Phillip A. B. Galli, Juana L. Rivera, Gisela N. Ortiz-León, Cesar Briceno, Marina Kounkel, Lee Hartmann, Rosa M. Torres, John J. Tobin, Gerardo Pech
Publikováno v:
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), 834(2), 143
NASA Astrophysics Data System
NASA Astrophysics Data System
We report on new distances and proper motions to seven stars across the Serpens/Aquila complex. The observations were obtained as part of the Gould's Belt Distances Survey (GOBELINS) project between September 2013 and April 2016 with the Very Long Ba
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0bc318461b353c67cc85962e413bdc38
http://iopscience.iop.org/article/10.3847/1538-4357/834/2/143/meta
http://iopscience.iop.org/article/10.3847/1538-4357/834/2/143/meta
Autor:
Luis F. Rodríguez, Gisela N. Ortiz-León, S. A. Dzib, Laurent Loinard, Rosa M. Torres, John J. Tobin, Lee Hartmann, Cesar Briceno, Neal J. Evans, Amy J. Mioduszewski, Gerardo Pech, Marina Kounkel, Andrew F. Boden, Phillip A. B. Galli, Juana L. Rivera
Publikováno v:
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), 834(2), 142
NASA Astrophysics Data System
NASA Astrophysics Data System
We present the results of the Gould's Belt Distances Survey (GOBELINS) of young star forming regions towards the Orion Molecular Cloud Complex. We detected 36 YSOs with the Very Large Baseline Array (VLBA), 27 of which have been observed in at least
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::80ef44cda371f4037f4da9af3aa5e19f
http://hdl.handle.net/1887/59417
http://hdl.handle.net/1887/59417
Publikováno v:
The Astrophysical Journal. 695:1527-1536
We have used interferometric and spectroscopic observations of HR 8257 to determine a three-dimensional orbit of the system. The orbit has a period of 12.21345 days and an eccentricity of 0.2895. The masses of the F0 and F2 dwarf components are 1.56
Autor:
Andrew F. Boden, A. Quirrenbach
Publikováno v:
Proceedings of the International Astronomical Union. 3:36-43
We review the status of ground-based interferometric astrometry. This will include a review of technology and results in differential techniques (e.g. relative orbit determination), as well as global astrometry techniques (globally-registered paralla
Autor:
William G. Bagnuolo, S. T. Ridgway, J. Sturmann, Andrew F. Boden, David H. Berger, Gerard van Belle, L. Sturmann, H. A. McAlister, R. R. Thompson, P. J. Goldfinger, T. ten Brummelaar, Neal J. Turner, David R. Ciardi
Publikováno v:
The Astrophysical Journal. 659:1623-1628
Using the CHARA Array and the Palomar Testbed Interferometer, the chemically peculiar star $\lambda$ Bo\"{o}tis has been spatially resolved. We have measured the limb darkened angular diameter to be $\theta_{LD} = 0.533\pm0.029$ mas, corresponding to