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From Wikipedia, the free encyclopedia

DG Tauri B
Image of DG Tau B obtained with the James Webb Space Telescope combining the F164N, F212N and F323N filters.

DG Tauri B, NASA, ESA, CSA, STSci, Delabrosse et al. 2024.
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 04h 27m 04.691s[1]
Declination +26° 06′ 16.04″[1]
Apparent magnitude (V) 10.50 (A)[2]
Astrometry
Parallax (π)8.2524 ± 0.1461 mas[1]
Distance395 ± 7 ly
(121 ± 2 pc)
Other designations
2MASS J04270469+2606163[3]
Database references
SIMBADDG Tau B cRN data

DG Tauri B, near the T Tauri star DG Tauri,[4] is a young stellar object located 450 light-years (140 parsecs) from Earth, within the Taurus constellation.[5] Observations of DG Tauri B were first made in October, and later December 1995 at the 6 element Owens Valley millimeter wave array.[6] Its most notable characteristics are its bipolar jets of molecular gas and dust emanating from either side of the object.[5][6] Red-shifted carbon monoxide emissions extend out 6,000 AU to the northwest of the object from the undetermined source, and are symmetrically distributed about the jet, while blue-shifted CO emissions are confined to a region with a roughly 500 AU radius.[6]

References

  1. ^ a b c Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
  2. ^ Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
  3. ^ "V* DG Tau". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 29 September 2018.
  4. ^ Varga, J; Gabányi, K. É; Ábrahám, P; Chen, L; Kóspál, Á; Menu, J; Ratzka, Th; Van Boekel, R; Dullemond, C. P; Henning, Th; Jaffe, W; Juhász, A; Moór, A; Mosoni, L; Sipos, N (2017). "Mid-infrared interferometric variability of DG Tauri: Implications for the inner-disk structure". Astronomy & Astrophysics. 604: A84. arXiv:1704.05675. doi:10.1051/0004-6361/201630287. S2CID 119475529.
  5. ^ a b "Disk Around Young Star. A View of DG Tauri B". www.spacetelescope.org.
  6. ^ a b c Mitchell, George F; Sargent, Anneila I; Mannings, Vincent (1997). "DG Tauri B: The Interaction of an Atomic Jet with Ambient Molecular Gas". The Astrophysical Journal. 483 (2): L127–L130. Bibcode:1997ApJ...483L.127M. doi:10.1086/310750.


This page was last edited on 16 April 2024, at 09:46
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