HD 283572 – Wikipedia

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Young star in constellation Taurus

HD 283572 is a young T Tauri-type pre-main sequence star in the constellation of Taurus about 414 light years away, belonging to the Taurus Molecular Cloud.[3] It is a rather evolved protostar which already dispersed its birth shroud.[4] The star emits a very high X-ray flux of 1031 ergs/s. That radiation flux associated with the magnetic activity induced a high coronal temperature of 3 kEv and regular flares.[6] HD 283572 will eventually evolve to an A-type main-sequence star when on the main sequence.[3] It is no longer accreting mass, and is magnetically decoupled from the remnants of the protoplanetary disk,[3] belonging to the terminal, 3rd phase of the disk evolution.[7]

Protoplanetary system[edit]

HD 283572 is surrounded by a light (<0.0004 M☉) and faint protoplanetary disk with uncertain inclination. Different instruments yielded measurements of disk inclination to the plane of sky from 35 to 60 degrees.[7] A search for planetary transits was performed but no planets were detected as of 2019.[8]

References[edit]

  1. ^ Strassmeier, K. G.; Rice, J. B. (November 1998). “Doppler imaging of stellar surface structure. IX. A high-resolution image of the weak-lined T Tauri star HDE 283572 = V987 Tauri”. Astronomy and Astrophysics. 339: 497–506. Bibcode:1998A&A…339..497S. Retrieved 8 April 2022.
  2. ^ a b c d e “HD 283572”. SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-11-01.
  3. ^ a b c d e f g Scelsi, L.; Maggio, A.; Peres, G.; Pallavicini, R. (2005), “Coronal properties of G-type stars in different evolutionary phases”, Astronomy & Astrophysics, 432 (2): 671–685, arXiv:astro-ph/0501631, Bibcode:2005A&A…432..671S, doi:10.1051/0004-6361:20041739, S2CID 15298988
  4. ^ a b c d e Torres, Rosa M.; Loinard, Laurent; Mioduszewski, Amy J.; Rodriguez, Luis F. (2007), “VLBA Determination of the Distance to Nearby Star‐forming Regions. II. Hubble 4 and HDE 283572 in Taurus”, The Astrophysical Journal, 671 (2): 1813–1819, arXiv:0708.4403, Bibcode:2007ApJ…671.1813T, doi:10.1086/522924, S2CID 16357104
  5. ^ a b c Brown, A. G. A.; et al. (Gaia collaboration) (2021). “Gaia Early Data Release 3: Summary of the contents and survey properties”. Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A…649A…1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  6. ^ Favata, F.; Micela, G.; Sciortino, S. (1998), “X-ray spectroscopy of the weak-lined T Tauri star HD 283572”, Astronomy and Astrophysics, 336: 413–420, Bibcode:1998A&A…337..413F
  7. ^ a b Yasui, Chikako; Hamano, Satoshi; Fukue, Kei; Kondo, Sohei; Sameshima, Hiroaki; Takenaka, Keiichi; Matsunaga, Noriyuki; Ikeda, Yuji; Kawakita, Hideyo; Otsubo, Shogo; Watase, Ayaka; Taniguchi, Daisuke; Mizumoto, Misaki; Izumi, Natsuko; Kobayashi, Naoto (2019), “Possible Progression of Mass-flow Processes around Young Intermediate-mass Stars Based on High-resolution Near-infrared Spectroscopy. I. Taurus”, The Astrophysical Journal, 886 (2): 115, arXiv:1909.09850, Bibcode:2019ApJ…886..115Y, doi:10.3847/1538-4357/ab45ee, S2CID 202718804
  8. ^ Hambálek, Ľ.; Vaňko, M.; Paunzen, E.; Smalley, B. (2019), “T Tauri stars in the SuperWASP and NSVS surveys”, Monthly Notices of the Royal Astronomical Society, 483 (2): 1642–1654, arXiv:1811.08655, Bibcode:2019MNRAS.483.1642H, doi:10.1093/mnras/sty3151


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