From Wikipedia, the free encyclopedia
τ Ophiuchi
Location of τ Ophiuchi (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Ophiuchus
Right ascension 18h 03m 04.91992s [1]
Declination −8° 10′ 49.2586″ [1]
Apparent magnitude (V) 5.24 (A) / 5.94 (B) [2]
Characteristics
Spectral type F2V(A) / F5V (B) [2]
U−B color index +0.05 (A) [3]
B−V color index +0.38 (A) [3]
Astrometry
Radial velocity (Rv)-38.39 [4] km/s
Proper motion (μ) RA: +15.78 [1]  mas/ yr
Dec.: -37.79 [1]  mas/ yr
Parallax (π)19.48 ± 0.66  mas [1]
Distance167 ± 6  ly
(51 ± 2  pc)
Details
Mass1.54 (A) / 1.29 (B) [5]  M
Surface gravity (log g)4.18 (A) [6]  cgs
Temperature6,813 (A) [6]  K
Other designations
BD-08°4549, CCDM J18031-0811AB, 69 Ophiuchi, HIP 88404, HD 164764+164765, HR 6733+6734, WDS J18031-0811AB
Database references
SIMBAD data

Tau Ophiuchi (τ Oph) is a multiple star in the constellation Ophiuchus, approximately 167 light years away based on parallax. [1] Its two main components are two yellow-white main sequence stars, A, of magnitude 5.24 and class F2V, and B, of magnitude 5.94 and class F5V, [2] orbiting each other with a period of 257 years and eccentricity around 0.77. [7] A is reported as a spectroscopic binary with a smaller star of 0.29 solar masses orbiting it every 186 days. [5] An additional component, C, has a separation of 100.8" and magnitude 11.28. [8]

References

  1. ^ a b c d e f Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv: 0708.1752. Bibcode: 2007A&A...474..653V. doi: 10.1051/0004-6361:20078357. S2CID  18759600. Vizier catalog entry
  2. ^ a b c Hoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H. 5050. Bibcode: 1995yCat.5050....0H.
  3. ^ a b Mallama, A. (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers. 42 (2): 443. Bibcode: 2014JAVSO..42..443M.
  4. ^ Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.; Morrell, N. I.; Torres, G.; Udry, S. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics. 424 (2): 727–732. arXiv: astro-ph/0406573. Bibcode: 2004A&A...424..727P. doi: 10.1051/0004-6361:20041213. S2CID  119387088.
  5. ^ a b Tokovinin, A. (2008). "Comparative statistics and origin of triple and quadruple stars". Monthly Notices of the Royal Astronomical Society. 389 (2): 925–938. arXiv: 0806.3263. Bibcode: 2008MNRAS.389..925T. doi: 10.1111/j.1365-2966.2008.13613.x. S2CID  16452670.
  6. ^ a b David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal. 804 (2): 146. arXiv: 1501.03154. Bibcode: 2015ApJ...804..146D. doi: 10.1088/0004-637X/804/2/146. S2CID  33401607. Vizier catalog entry
  7. ^ Malkov, O. Yu.; Tamazian, V. S.; Docobo, J. A.; Chulkov, D. A. (2012). "Dynamical masses of a selected sample of orbital binaries". Astronomy & Astrophysics. 546: A69. Bibcode: 2012A&A...546A..69M. doi: 10.1051/0004-6361/201219774. Vizier catalog entry
  8. ^ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920. Vizier catalog entry


From Wikipedia, the free encyclopedia
τ Ophiuchi
Location of τ Ophiuchi (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Ophiuchus
Right ascension 18h 03m 04.91992s [1]
Declination −8° 10′ 49.2586″ [1]
Apparent magnitude (V) 5.24 (A) / 5.94 (B) [2]
Characteristics
Spectral type F2V(A) / F5V (B) [2]
U−B color index +0.05 (A) [3]
B−V color index +0.38 (A) [3]
Astrometry
Radial velocity (Rv)-38.39 [4] km/s
Proper motion (μ) RA: +15.78 [1]  mas/ yr
Dec.: -37.79 [1]  mas/ yr
Parallax (π)19.48 ± 0.66  mas [1]
Distance167 ± 6  ly
(51 ± 2  pc)
Details
Mass1.54 (A) / 1.29 (B) [5]  M
Surface gravity (log g)4.18 (A) [6]  cgs
Temperature6,813 (A) [6]  K
Other designations
BD-08°4549, CCDM J18031-0811AB, 69 Ophiuchi, HIP 88404, HD 164764+164765, HR 6733+6734, WDS J18031-0811AB
Database references
SIMBAD data

Tau Ophiuchi (τ Oph) is a multiple star in the constellation Ophiuchus, approximately 167 light years away based on parallax. [1] Its two main components are two yellow-white main sequence stars, A, of magnitude 5.24 and class F2V, and B, of magnitude 5.94 and class F5V, [2] orbiting each other with a period of 257 years and eccentricity around 0.77. [7] A is reported as a spectroscopic binary with a smaller star of 0.29 solar masses orbiting it every 186 days. [5] An additional component, C, has a separation of 100.8" and magnitude 11.28. [8]

References

  1. ^ a b c d e f Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv: 0708.1752. Bibcode: 2007A&A...474..653V. doi: 10.1051/0004-6361:20078357. S2CID  18759600. Vizier catalog entry
  2. ^ a b c Hoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H. 5050. Bibcode: 1995yCat.5050....0H.
  3. ^ a b Mallama, A. (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers. 42 (2): 443. Bibcode: 2014JAVSO..42..443M.
  4. ^ Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.; Morrell, N. I.; Torres, G.; Udry, S. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics. 424 (2): 727–732. arXiv: astro-ph/0406573. Bibcode: 2004A&A...424..727P. doi: 10.1051/0004-6361:20041213. S2CID  119387088.
  5. ^ a b Tokovinin, A. (2008). "Comparative statistics and origin of triple and quadruple stars". Monthly Notices of the Royal Astronomical Society. 389 (2): 925–938. arXiv: 0806.3263. Bibcode: 2008MNRAS.389..925T. doi: 10.1111/j.1365-2966.2008.13613.x. S2CID  16452670.
  6. ^ a b David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal. 804 (2): 146. arXiv: 1501.03154. Bibcode: 2015ApJ...804..146D. doi: 10.1088/0004-637X/804/2/146. S2CID  33401607. Vizier catalog entry
  7. ^ Malkov, O. Yu.; Tamazian, V. S.; Docobo, J. A.; Chulkov, D. A. (2012). "Dynamical masses of a selected sample of orbital binaries". Astronomy & Astrophysics. 546: A69. Bibcode: 2012A&A...546A..69M. doi: 10.1051/0004-6361/201219774. Vizier catalog entry
  8. ^ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode: 2001AJ....122.3466M. doi: 10.1086/323920. Vizier catalog entry



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