Arid
DOI10.1093/mnras/staa3834
Planet formation in intermediate-separation binary systems
Panic, O.; Haworth, T. J.; Petr-Gotzens, M. G.; Miley, J.; van den Ancker, M.; Vioque, M.; Siess, L.; Parker, R.; Clarke, C. J.; Kamp, I; Kennedy, G.; Oudmaijer, R. D.; Pascucci, I; Richards, A. M. S.; Ratzka, T.; Qi, C.
通讯作者Panic, O (corresponding author), Univ Leeds, Sch Phys & Astron, Leeds LS2 9JT, W Yorkshire, England.
来源期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
EISSN1365-2966
出版年2021
卷号501期号:3页码:4317-4328
英文摘要We report the first characterization of the individual discs in the intermediate-separation binary systems KK Oph and HD 144668 at millimetre wavelengths. In both systems, the circumprimary and the circumsecondary discs are detected in the millimetre continuum emission, but not in (CO)-C-13 nor (CO)-O-18 lines. Even though the disc structure is only marginally resolved, we find indications of large-scale asymmetries in the outer regions of the primary discs, most likely due to perturbation by the companion. The derived dust masses are firmly above debris disc level for all stars. The primaries have about three times more dust in their discs than the secondaries. In the case of HD 144668, the opacity spectral index of the primary and secondary differ by a large margin of 0.69, which may be a consequence of the secondary disc being more compact. Upper limits on the gas masses imply less than 0.1 M-jup in any of these discs, meaning that giant planets can no longer form in them. Considering that there have been no massive gas discs identified to date in intermediate-separation binaries (i.e. binaries at a few hundred au separation), this opens space for speculation whether their binarity causes the removal of gas, with tidal interaction truncating the discs and hence shortening the accretion time-scale. More systematic studies in this respect are sorely needed.
英文关键词planets and satellites: formation protoplanetary discs stars: pre-main-sequence (stars:) binaries: visual stars: variables: T Tauri, Herbig Ae/Be submillimetre: planetary systems techniques: interferometric
类型Article
语种英语
开放获取类型Green Published, Green Accepted, Green Submitted
收录类别SCI-E
WOS记录号WOS:000686047600017
WOS关键词HERBIG-AE/BE STARS ; FIELD EXTINCTION MAPS ; BROWN DWARF DESERT ; PROTOPLANETARY DISKS ; GIANT PLANETS ; DM-TAU ; ACCRETION ; MASS ; CIRCUMSTELLAR ; SUBMILLIMETER
WOS类目Astronomy & Astrophysics
WOS研究方向Astronomy & Astrophysics
来源机构University of Arizona ; University of London
资源类型期刊论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/364197
作者单位[Panic, O.; Miley, J.; Vioque, M.; Oudmaijer, R. D.] Univ Leeds, Sch Phys & Astron, Leeds LS2 9JT, W Yorkshire, England; [Haworth, T. J.] Queen Mary Univ London, Sch Phys & Astron, Astron Unit, London E1 4NS, England; [Petr-Gotzens, M. G.; van den Ancker, M.] European Southern Observ Headquarters, Karl Schwatzschild Str 2, D-85748 Garching, Germany; [Petr-Gotzens, M. G.] Ludwig Maximilians Univ Munchen, Univ Sternwarte, Scheinerstr 1, D-81679 Munich, Germany; [Miley, J.; Vioque, M.] Joint ALMA Observ, Alonso Cordova 3107, Santiago 7630355, Chile; [Siess, L.] Univ Libre Bruxelles ULB, Inst Astron & Astrophys, CP 226, B-1060 Brussels, Belgium; [Parker, R.] Univ Sheffield, Dept Phys & Astron, Hicks Bldg,Hounsfield Rd, Sheffield S3 7RH, S Yorkshire, England; [Clarke, C. J.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England; [Kamp, I] Univ Groningen, Kapteyn Astron Inst, POB 72, NL-9700 AB Groningen, Netherlands; [Kennedy, G.] Univ Warwick, Dept Phys, Gibbet Hill Rd, Coventry CV4 7AL, W Mid...
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Panic, O.,Haworth, T. J.,Petr-Gotzens, M. G.,et al. Planet formation in intermediate-separation binary systems[J]. University of Arizona, University of London,2021,501(3):4317-4328.
APA Panic, O..,Haworth, T. J..,Petr-Gotzens, M. G..,Miley, J..,van den Ancker, M..,...&Qi, C..(2021).Planet formation in intermediate-separation binary systems.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,501(3),4317-4328.
MLA Panic, O.,et al."Planet formation in intermediate-separation binary systems".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 501.3(2021):4317-4328.
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