Access the full text.
Sign up today, get DeepDyve free for 14 days.
Loading next page...
/lp/springer-journals/physical-and-geometric-parameters-of-the-evolved-binary-system-hd-6009-t04G7eS60N
References (38)
-
E. Horch, S. Robinson, R. Meyer, W. Altena, Z. Ninkov, Albert Piterman (2002)
Speckle Observations of Binary Stars with the WIYN Telescope. II. Relative Astrometry Measures during 1998-2000The Astronomical Journal, 123
-
M. Perryman (2008)
Astronomical Applications of Astrometry: The Hipparcos and Tycho Catalogues -
A. Tutukov (1998)
Planets and starsAstronomy Reports
-
Depending on the parameters of the system’s components and their positions on the evolutionary tracks -
The entire and individual UBV R Johnson-Cousins, uvby Str¨omgren and BV Tycho synthetic magnitudes and colors of the system were calculated -
C. Sterken (2007)
The Future of Photometric, Spectrophotometric and Polarimetric Standardization, 364
-
The estimated parameters show a good consistency with the previously published ones -
E. Horch, R. Meyer, W. Altena (2004)
Speckle Observations of Binary Stars with the WIYN Telescope. IV. Differential PhotometryThe Astronomical Journal, 127
-
M. Al-Wardat (2003)
Spectral energy distributions and model atmosphere parameters of the binary systems COU1289 and COU1291 -
M. Al-Wardat, Y. Balega, V. Leushin, V. Leushin, N. Yusuf, Ali Taani, K. Al-Waqfi, S. Masda (2014)
Speckle interferometric binary system HD375; Is it a sub-giant binary?Astrophysical Bulletin, 69
-
E. Horch, W. Altena, William Cyr, Lori Kinsman-Smith, Amit Srivastava, Jing Zhou (2008)
CHARGE-COUPLED DEVICE SPECKLE OBSERVATIONS OF BINARY STARS WITH THE WIYN TELESCOPE. V. MEASURES DURING 2001–2006The Astronomical Journal, 136
-
M. Al-Wardat, H. Widyan, Ahmed Al-thyabat (2013)
Complex Analysis of the Stellar Binary HD25811: A Subgiant SystemPublications of the Astronomical Society of Australia, 31
-
K. Yoss (1961)
Spectral and Luminosity Classifications and Measurements of the Strength of Cyanogen Absorption for Late-Type Stars from Objective-Prism Spectra.The Astrophysical Journal, 134
-
B. Mason, W. Hartkopf, D. Gies, T. Henry, J. Helsel (2008)
THE HIGH ANGULAR RESOLUTION MULTIPLICITY OF MASSIVE STARSThe Astronomical Journal, 137
-
D. Gray (2021)
The Observation and Analysis of Stellar Photospheres -
(1961)
Yoss, Astrophys -
M. Al-Wardat (2008)
Synthetic photometry of speckle interferometric binariesAstrophysical Bulletin, 63
-
E. Schlafly, D. Finkbeiner (2010)
MEASURING REDDENING WITH SLOAN DIGITAL SKY SURVEY STELLAR SPECTRA AND RECALIBRATING SFDThe Astrophysical Journal, 737
-
T. Polk, S. Turner, Ieca Hoffman, Polk
Internet Engineering Task Force (ietf) Security Considerations for the Sha-0 and Sha-1 Message-digest Algorithms Sha-0 and Sha-1 Security Consideration -
P. Natarajan, R. Crittenden, U. Pen, T. Theuns (2001)
Publications of the Astronomical Society of Australia -
(2005)
Accepted for publication in the Astronomical Journal A recalibration of optical photometry: -
E. Horch, David Falta, Lisa Anderson, Michael DeSousa, Craig Miniter, Tasmia Ahmed, W. Altena (2009)
CCD SPECKLE OBSERVATIONS OF BINARY STARS WITH THE WIYN TELESCOPE. VI. MEASURES DURING 2007–2008The Astronomical Journal, 139
-
M. Al-Wardat (2012)
Physical Parameters of the Visually Close Binary Systems Hip70973 and Hip72479Publications of the Astronomical Society of Australia, 29
-
B. Mason, Christian Martin, W. Hartkopf, D. Barry, M. Germain, G. Douglass, C. Worley, G. Wycoff, T. Brummelaar, O. Franz (1999)
Speckle Interferometry of New and Problem Hipparcos BinariesThe Astronomical Journal, 117
-
(1961)
K . M . Yoss -
parameters of the system’s components were estimated depending on the best fit between the observational SED and synthetic ones built using the atmospheric modeling of the individual components -
I. Balega, Y. Balega, A. Maksimov, E. Malogolovets, D. Rastegaev, Z. Shkhagosheva, G. Observatory, Russia, Max Radioastronomie, Germany (2007)
Speckle interferometry of nearby multiple stars. IV. Measurements in 2004 and new orbitsAstrophysical Bulletin, 62
-
K. Lang (1992)
Astrophysical Data : Planets and Stars -
I. Bonnell (1994)
A new binary formation mechanismMonthly Notices of the Royal Astronomical Society, 269
-
M. Al-Wardat (2009)
Parameters of the components of visually close binary systems: Hip 11352Astronomische Nachrichten, 330
-
(2001)
IAU Symposium, Vol. 200 -
M. Al-Wardat, H. Widyan, H. Widyan (2009)
Parameters of the visually close binary system Hip11253 (HD14874)Astrophysical Bulletin, 64
-
L. Girardi, A. Bressan, G. Bertelli, C. Chiosi (1999)
Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 , and from to 0.03Astronomy & Astrophysics Supplement Series, 141
-
E. Horch, Lizzie Bahi, Joseph Gaulin, S. Howell, W. Sherry, Roberto Gallé, W. Altena (2010)
SPECKLE OBSERVATIONS OF BINARY STARS WITH THE WIYN TELESCOPE. VII. MEASURES DURING 2008–2009The Astronomical Journal, 143
-
I. Balega, Y. Balega, A. Maksimov, E. Pluzhnik, D. Schertl, Z. Shkhagosheva, G. Weigelt (2002)
Speckle interferometry of nearby multiple stars. II.Astronomy and Astrophysics, 422
-
A modification to the parallax of the system is introduced within the error of Hipparcos parallax measurement -
E. Horch, S. Gomez, W. Sherry, S. Howell, D. Ciardi, Lisa Anderson, W. Altena (2011)
OBSERVATIONS OF BINARY STARS WITH THE DIFFERENTIAL SPECKLE SURVEY INSTRUMENT. II. HIPPARCOS STARS OBSERVED IN 2010 JANUARY AND JUNEThe Astronomical Journal, 141
-
E. Pluzhnik (2005)
Differential photometry of speckle-interferometric binary and multiple starsAstronomy and Astrophysics, 431
- Publisher
- Springer Journals
- Copyright
- Copyright © 2014 by Pleiades Publishing, Ltd.
- Subject
- Physics; Astronomy, Astrophysics and Cosmology
- ISSN
- 1990-3413
- eISSN
- 1990-3421
- DOI
- 10.1134/S1990341314040075
- Publisher site
- See Article on Publisher Site
Abstract
Atmospheric modeling and dynamical analysis of the components of the speckle interferometric binary system HD 6009 were used to estimate their individual physical and geometric parameters. Model atmospheres were constructed using a grid of Kurucz’s solar metallicity blanketed models and used to compute the individual synthetic spectral energy distribution (SED) for each component separately. These SEDs were combined together to compute the entire SED for the system from the net luminosities of the components A and B located at a distance d from the Earth. We used the modified feedback parameters and the iteration method to get the best fit between the synthetic and observed total SEDs. The physical and geometric parameters of the system’s components were derived as T eff A = 5625 ± 75 K, T eff B = 5575 ± 75 K, log g A = 3.75 ± 0.25, log g B = 3.75 ± 0.25, R A = 2.75 ± 0.30R ⊙, R B = 2.65 ± 0.30 R ⊙, $$M_V^A = 2.^m 99 \pm 0.30$$ , $$M_V^B = 3.^m 12 \pm 0.30$$ , M A = 1.60 ± 0.20 M ⊙, M B = 1.46 ± 0.20 M ⊙, L A = 15.84 ± 1.60 L ⊙, and L B = 15.83 ± 1.60 L ⊙, with G6 spectral types for both components.
Journal
Astrophysical Bulletin – Springer Journals
Published: Nov 23, 2014