Astronomy:CQ Tauri

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Short description: Star in the constellation Taurus
CQ Tauri
CQTauLightCurve.png
A visual band light curve for CQ Tauri, plotted from INTEGRAL OMC data[1]
Observation data
Equinox J2000.0]] (ICRS)
Constellation Taurus
Right ascension  05h 35m 58.467s[2]
Declination 24° 44′ 54.09″[2]
Apparent magnitude (V) 10.48[3] (8.7 to 12.25)[4]
Characteristics
Evolutionary stage Pre-main-sequence[5]
Spectral type F5IVe[6]
B−V color index 0.696±0.091[3]
Variable type Orion variable[4]
Astrometry
Radial velocity (Rv)22.60±2.7[7] km/s
Proper motion (μ) RA: 2.987[2] mas/yr
Dec.: −26.364[2] mas/yr
Parallax (π)6.6946 ± 0.0600[2] mas
Distance487 ± 4 ly
(149 ± 1 pc)
Absolute magnitude (MV)5.92[8]
Details
Mass1.67[9] M☉
Radius1.7[10] R☉
Luminosity10[9] L☉
Surface gravity (log g)4.0[8] cgs
Temperature6,900[9] K
Metallicity [Fe/H]+0.14[11] dex
Rotational velocity (v sin i)105.0±5.0[6] km/s
Age10[9] Myr
Other designations
CQ Tau, BD+24°873, HD 36910, HIP 26295, SAO 77299, PPM 94541[12]
Database references
SIMBADdata

CQ Tauri is a young variable star[5] in the equatorial constellation of Taurus. It is too faint to be visible to the naked eye with an apparent visual magnitude that ranges from 8.7 to 12.25.[4] The distance to this star is approximately 487 light years based on parallax measurements, and it is drifting further away with a radial velocity of ~23 km/s.[7] It appears to be part of the T-association Tau 4.[8] CQ Tauri lies close enough to the ecliptic to undergo lunar occultations.[13]

This star was independently reported as a variable by Artjukinov (sp?) in 1948 and C. Hoffmeister in 1949.[14] Hoffmeister classified it as a member of the RW Aurigae-like variables with a brightness that ranged from an apparent visual magnitude of 8.7 down to 10.5,[15] making it one of the brightest members of that type.[14] G. H. Herbig in 1960 found a spectral class of F2 for this star,[16] and by 1973 it was classed as an Orion variable of the T Tauri type.[17] In 1968, W. Götz and W. Wenzel discovered a faint emission of blue light coming from the system.[18]

Spectral images of the system in 1973 showed double emission lines on an F-type star.[19] It was found to be an infrared source by IRAS and associated with nebulosity, which allowed it to be cataloged as a Herbig Ae/Be star in 1994 by P. S. Thé and associates.[20] The star undergoes irregular brightness decreases that are otherwise similar to an Algol-like variation. It is being orbited by an inhomogeneous accretion disk, which is the source for the emission lines.[21]

CQ Tauri is a pre-main-sequence star with a stellar classification of F5IVe.[6] It has 1.67 times the mass of the Sun and is radiating 10 times the Sun's luminosity with an effective temperature of 6,900 K. The star is about 10 million years old[9] and is spinning with a projected rotational velocity of 105 km/s.[6] Simulations intended to reproduce the distribution of the circumstellar disk suggest an embedded planet with a mass of 6–9 Jupiter mass is orbiting the star at a distance of ~20 AU.[9] Near infrared observations in 2018 show a spiral structure in the disk that is consistent with the presence of an orbiting planet. However, no planet was detected.[22]

Protoplanetary system

Observations with the Very Large Array during 2000 demonstrated the extent of the massive protoplanetary disk orbiting the star. The mass of dust in the disk was estimated at 1.5×10−4 M☉.[23] Measurements suggest the dust grains in the disk around CQ Tauri have grown to a maximum of about a centimetre in size,[24] with decreasing grain size beyond 40 astronomical unit|AU from the host star.[25] Data from the Atacama Large Millimeter Array show a cavity in the inner disk that is depleted of gas and dust.[9] Isolated, thick clouds of dust are randomly obscuring the star.[26]

In 2022, four spiral arms were detected in the protoplanetary disk. An as yet unseen planet on an eccentric and inclined orbit is suspected to be disturbing the shape of the disk.[27]

References

  1. ↑ "OMC Archive". The Astronomical Data Centre at CAB. https://sdc.cab.inta-csic.es/omc/secure/form_busqueda.jsp?resetForm=true. 
  2. ↑ 2.0 2.1 2.2 2.3 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G.  Gaia EDR3 record for this source at VizieR.
  3. ↑ 3.0 3.1 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A. 
  4. ↑ 4.0 4.1 4.2 Samus, N. N. et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1 61 (1): 80–88, doi:10.1134/S1063772917010085, Bibcode: 2017ARep...61...80S. 
  5. ↑ 5.0 5.1 Testi, L. et al. (May 2003), "Large grains in the disk of CQ Tau", Astronomy and Astrophysics 403: 323–328, doi:10.1051/0004-6361:20030362, Bibcode: 2003A&A...403..323T. 
  6. ↑ 6.0 6.1 6.2 6.3 Mora, A. et al. (2001), "EXPORT: Spectral classification and projected rotational velocities of Vega-type and pre-main sequence stars", Astronomy & Astrophysics 378 (1): 116–131, doi:10.1051/0004-6361:20011098, Bibcode: 2001A&A...378..116M. 
  7. ↑ 7.0 7.1 Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system", Astronomy Letters 32 (11): 759–771, doi:10.1134/S1063773706110065, Bibcode: 2006AstL...32..759G. 
  8. ↑ 8.0 8.1 8.2 Alecian, E. et al. (February 2013), "A high-resolution spectropolarimetric survey of Herbig Ae/Be stars - I. Observations and measurements", Monthly Notices of the Royal Astronomical Society 429 (2): 1001–1026, doi:10.1093/mnras/sts383, Bibcode: 2013MNRAS.429.1001A. 
  9. ↑ 9.0 9.1 9.2 9.3 9.4 9.5 9.6 Giulia Ubeira Gabellini, M. et al. (July 2019), "A dust and gas cavity in the disc around CQ Tau revealed by ALMA", Monthly Notices of the Royal Astronomical Society 486 (4): 4638–4654, doi:10.1093/mnras/stz1138, Bibcode: 2019MNRAS.486.4638U. 
  10. ↑ Stassun, Keivan G. et al. (September 9, 2019), "The Revised TESS Input Catalog and Candidate Target List", The Astronomical Journal 158 (4): 138, doi:10.3847/1538-3881/ab3467, ISSN 0004-6256, Bibcode: 2019AJ....158..138S. 
  11. ↑ Bochanski, John J. et al. (March 13, 2018), "Fundamental Properties of Co-moving Stars Observed by Gaia", The Astronomical Journal 155 (4): 149, doi:10.3847/1538-3881/aaaebe, ISSN 0004-6256, Bibcode: 2018AJ....155..149B. 
  12. ↑ "CQ Tau". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=CQ+Tau. 
  13. ↑ Cassar, L. et al. (March 1989), "Lunar Occultations of IRAS Point Sources, 1991--2000", Astrophysical Journal Supplement 69: 651, doi:10.1086/191323, Bibcode: 1989ApJS...69..651C.  See table p. 658, IRAS 05328+2443.
  14. ↑ 14.0 14.1 Ashbrook, J. (August 1950), "HD 36910: a bright variable of the RW Aurigae type", Astronomical Journal 55: 148, doi:10.1086/106374, Bibcode: 1950AJ.....55..148A. 
  15. ↑ Hoffmeister, Cuno (November 1949), "Die RW Aurigae-Sterne und ihre Nebenformen" (in de), Astronomische Nachrichten 278: 24, doi:10.1002/asna.19492780102, Bibcode: 1949AN....278...24H.  Listed as "S 3942 Tau".
  16. ↑ Herbig, G. H. (May 1960), "Spectral Classifications for 112 Variable Stars", Astrophysical Journal 131: 632, doi:10.1086/146876, Bibcode: 1960ApJ...131..632H. 
  17. ↑ Cohen, M. (1973), "Infra-red observations of young stars - II. T Tauri stars and the Orion population", Monthly Notices of the Royal Astronomical Society 161: 97, doi:10.1093/mnras/161.1.97, Bibcode: 1973MNRAS.161...97C. 
  18. ↑ Berdyugin, A. V. et al. (August 1990), "Discovery of high linear polarization at brightness minima of CQ Tau", Astronomicheskii Zhurnal 67: 812, Bibcode: 1990AZh....67..812B. 
  19. ↑ Herbig, G. H.; Bell, K. Robbin (Jun 1988), "Third Catalog of Emission-Line Stars of the Orion Population", Lick Observatory Bulletin (Santa Cruz) 1111, Bibcode: 1988cels.book.....H. 
  20. ↑ The, P. S. et al. (April 1994), "A new catalogue of members and candidate members of the Herbig Ae/Be (HAEBE) stellar group", Astronomy and Astrophysics Supplement 104: 315–339, Bibcode: 1994A&AS..104..315T. 
  21. ↑ Kozlova, O. V. et al. (January 2000), "The Accretion Activity of the Ae Herbig Star CQ Tau", Astronomy Reports 44 (1): 36–44, doi:10.1134/1.163821, Bibcode: 2000ARep...44...36K. 
  22. ↑ Uyama, Taichi et al. (March 2020), "Near-infrared Imaging of a Spiral in the CQ Tau Disk", The Astronomical Journal 159 (3): 9, doi:10.3847/1538-3881/ab7006, 118, Bibcode: 2020AJ....159..118U. 
  23. ↑ Testi, L. et al. (June 2001), "Constraints on Properties of the Protoplanetary Disks around UX Orionis and CQ Tauri", The Astrophysical Journal 554 (2): 1087–1094, doi:10.1086/321406, Bibcode: 2001ApJ...554.1087T. 
  24. ↑ Banzatti, A. et al. (January 2011), "New constraints on dust grain size and distribution in CQ Tauri", Astronomy and Astrophysics 525: A12, doi:10.1051/0004-6361/201015206, A12, Bibcode: 2011A&A...525A..12B. 
  25. ↑ Trotta, F. et al. (October 2013), "Constraints on the radial distribution of the dust properties in the CQ Tauri protoplanetary disk", Astronomy & Astrophysics 558: A64, doi:10.1051/0004-6361/201321896, A64, Bibcode: 2013A&A...558A..64T. 
  26. ↑ Dodin, A. V.; Suslina, E. A. (June 2021), "Inhomogeneous dust eclipses in young stars: the case of CQ Tauri", Monthly Notices of the Royal Astronomical Society 503 (4): 5704–5714, doi:10.1093/mnras/stab487, Bibcode: 2021MNRAS.503.5704D. 
  27. ↑ Hammond, Iain; Christiaens, Valentin; Price, Daniel J.; Ubeira-Gabellini, Maria Giulia; Baird, Jennifer; Calcino, Josh; Benisty, Myriam; Lodato, Giuseppe et al. (2022), "External or internal companion exciting the spiral arms in CQ Tau?", Monthly Notices of the Royal Astronomical Society 515 (4): 6109–6121, doi:10.1093/mnras/stac2119 

Further reading

  • Safonov, Boris S. et al. (January 2022), "Apparent Motion of the Circumstellar Envelope of CQ Tau in Scattered Light", The Astronomical Journal 163 (1): 31, doi:10.3847/1538-3881/ac36cb, 31, Bibcode: 2022AJ....163...31S. 
  • Wölfer, L. et al. (April 2021), "A highly non-Keplerian protoplanetary disc. Spiral structure in the gas disc of CQ Tau", Astronomy & Astrophysics 648, doi:10.1051/0004-6361/202039469, A19, Bibcode: 2021A&A...648A..19W. 
  • Assani, K. (January 2020), "Variability in the Gas and Dust Emission of the UX Orioni Star CQ Tau", Bulletin of the American Astronomical Society 52 (1), Bibcode: 2020AAS...23545101A. 
  • Ubeira Gabellini, Maria Giulia (December 2018), "The gas and dust disk around the CQ Tau pre-main sequence star", Protoplanetary disks seen through the eyes of new-generation high-resolution instruments. Proceedings of the conference held 25–28 June 2018 in Rome, Italy: p. 30, doi:10.5281/zenodo.1893261, Bibcode: 2018ppd..confE..30U. 
  • Tax, Tomáš (November 2018), "Asymmetric CQ-Tau Transition Disk at High Angular Resolution", Take a Closer Look, 15–19 October 2018 in ESO-HQ, Garching b. München, Germany: p. 112, doi:10.5281/zenodo.1488994, Bibcode: 2018tcl..confE.112T. 
  • Shenavrin, V. I. et al. (May 2012), "Photometric activity of UX Ori stars and related objects in the near infrared and visual. BF Ori, CQ Tau, WW Vul, and SV Cep", Astronomy Reports 56 (5): 379–394, doi:10.1134/S1063772912040063, Bibcode: 2012ARep...56..379S. 
  • Chapillon, E. et al. (September 2010), "C I observations in the CQ Tauri proto-planetary disk: evidence of a very low gas-to-dust ratio?", Astronomy and Astrophysics 520: A61, doi:10.1051/0004-6361/201014841, A61, Bibcode: 2010A&A...520A..61C. 
  • Chapillon, E. et al. (November 2008), Charbonnel, C.; Combes, F.; Samadi, R., eds., "Disks around CQ Tau and MWC 758: Dense PDRs or gas dispersal?", SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics: p. 303, Bibcode: 2008sf2a.conf..303C. 
  • Kozlova, O. V. et al. (January 2007), "Structure of the inner region of the accretion disk of the Herbig Ae star CQ Tau based on long-term monitoring data", Astrophysics 50 (1): 26–39, doi:10.1007/s10511-007-0004-z, Bibcode: 2007Ap.....50...26K. 
  • Doucet, C. et al. (December 2006), "Mid-infrared imaging of the circumstellar dust around three Herbig Ae stars: HD 135344, CQ Tau, and HD 163296", Astronomy and Astrophysics 460 (1): 117–124, doi:10.1051/0004-6361:20054371, Bibcode: 2006A&A...460..117D. 
  • Shakhovskoj, D. N. et al. (April 2005), "Analysis of the Historical Light Curve of the UX Ori Star CQ Tau", Astrophysics 48 (2): 135–142, doi:10.1007/s10511-005-0014-7, Bibcode: 2005Ap.....48..135S. 
  • Shakhovskoy, D. N. et al. (2005), "Variations of Effective Size of Dust Grains in CQ Tau", Protostars and Planets V, Proceedings of the Conference held October 24–28, 2005, in Hilton Waikoloa Village, Hawai'i. LPI Contribution No. 1286 (1286): p. 8119, Bibcode: 2005prpl.conf.8119S. 
  • Minikulov, N. Kh. et al. (1993), "Investigation of light curves of young irregular variables. 1. SV CEP and CQ Tau", Astrofizika 36: 55–60, Bibcode: 1993Afz....36...55M. 
  • Polosukhina, N. S.; Lebedeva, L. (December 1966), "Polarization and Brightness Variations of the Magnetic Variable HD 215441", Soviet Astronomy 10: 407, Bibcode: 1966SvA....10..407P. 




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