List of transiting circumsecondary disks

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This is a list of transiting circumsecondary disks (including possible ring systems). A circumsecondary disk is a disk of gas and/or dust around a star, white dwarf or substellar object that is a secondary in a star system. In rare cases the system can be aligned in a way that makes it possible for the circumsecondary disk to transit in front of the primary. In some cases the observed dips can be so deep that researchers describe these dimming events as occultations.

Contents

The object J1407b was considered a circumsecondary disk in the past, but later turned out to be more likely a free-floating planetary-mass object with a disk. PDS 110 is a candidate with uncertain status, as later eclipses did not occur. VVV-WIT-07, [1] ASASSN-V J192543.72+402619.0, [2] ASASSN-21co, [3] FY Scuti, [4] OGLE-BLG182.1.162852, [5] and ZTF J185259.31+124955.2 [6] are candidates without much modelling of the disk.

List of transiting disks

Name of the primarySpectral type primarySecondary object classificationOrbital separation (AU)Orbital period (years)Disk radius (AU)Reference
Giant stars with possible mass transfer to the secondary in the past
TYC 2505-672-1 M2III B-type hot subdwarf 16.7–31.2 or 26.769.10.85–3.15 or 3.75 [7] [8]
Epsilon Aurigae F0II–III? B5V-star 18.1+1.2
−1.3		27.13.8+0.1
−0.4		 [9]
VVV-WIT-08 giant between K7 and M2object of unknown nature>11>0.25 [10]
Eta Geminorum M3.5 Ib-IIstar (about 2 M☉)7.88.2>0.75 [11]
Gaia17bpp M0IIIstar>6.51.4 [12]
EE Cephei B5III (Be star)star5.60.13 [13]
OGLE LMC-ECL-11893 B9III: (Be star)old low-mass object1.71.30.2 [14]
MWC 882 A0 (accretor, post-Algol variable)B7 (donor, post-RGB)0.530.200.28 (around primary) [15]
Young systems (secondary is star)
V773 Tauri binary: K3Ve (Li)binary star (two 1.5 M☉ stars)15.35±0.4526.55 [16]
Secondary possibly substellar object or planet
ASASSN-21js early-type starsubstellar object (brown dwarf or smaller)~13,000~610,0001.055 [17]
Gaia21bcv K4.5V (young star)low-mass star, brown dwarf or planet<225<33750.5 [18]
ASASSN-V J060000.76–310027.83 early K-dwarfobject of unknown nature~82~0.5 [19] [20]
EPIC 204376071 M5.3 (young star)about 3 MJ object>0.220.012 (2.60 R☉) [21] [22]
V928 Tauri M0.8 (young binary)substellar object with high mass (at least >50 MJ)<3.20.18–2.80.006 (1.39 R☉) [23] [22]
EPIC 220208795 early K-dwarf>1.5 MJ object1.20–1.44 (aphelion)0.65–0.800.005 (1.14 R☉) [22]
KIC 10403228 M0.88 or 1.44 RJ object4500.0012 or 0.0017 (2.6 or 3.7 RJ) [24]
Sun G2V Saturn (planet; included for comparison)9.5826 AU29.44750.00091 AU [lower-alpha 1] [25] [26] [27]
HIP 41378 late F-type star HIP 41378 f (12 ME planet, with radius of 3.7 R🜨 if it has rings)1.371.490.0004 (9.6 R🜨) [28]
K2-33 M dwarf (young star) K2-33b (planet)0.04090.015 (5.424 days)0.0002 (5 R🜨) [29]

See also

Notes

  1. ↑ Outer edge of Saturn's A ring.

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References

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  6. ↑ Bernhard, Klaus; Lloyd, Christopher (1 August 2024). "ZTF J185259.31+124955.2: A new evolved disc-eclipsing binary system". Astronomy and Astrophysics. 688: A58. arXiv: 2405.15555 . Bibcode:2024A&A...688A..58B. doi:10.1051/0004-6361/202450203. ISSN   0004-6361.
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  24. ↑ Aizawa, Masataka; Uehara, Sho; Masuda, Kento; Kawahara, Hajime; Suto, Yasushi (1 April 2017). "Toward Detection of Exoplanetary Rings via Transit Photometry: Methodology and a Possible Candidate". The Astronomical Journal. 153 (4): 193. arXiv: 1702.08252 . Bibcode:2017AJ....153..193A. doi: 10.3847/1538-3881/aa6336 . ISSN   0004-6256.
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  29. ↑ Ohno, Kazumasa; Thao, Pa Chia; Mann, Andrew W.; Fortney, Jonathan J. (25 November 2022). "A Circumplanetary Dust Ring May Explain the Extreme Spectral Slope of the 10 Myr Young Exoplanet K2-33b". The Astrophysical Journal Letters. 940 (2): L30. arXiv: 2211.07706 . Bibcode:2022ApJ...940L..30O. doi: 10.3847/2041-8213/ac9f3f . ISSN   2041-8205.
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