Imaging the Inner Astronomical Unit of Herbig Be Star HD 190073
dc.contributor.author | Ibrahim, N | |
dc.contributor.author | Monnier, JD | |
dc.contributor.author | Kraus, S | |
dc.contributor.author | Le Bouquin, J-B | |
dc.contributor.author | Anugu, N | |
dc.contributor.author | Baron, F | |
dc.contributor.author | ten Brummelaar, T | |
dc.contributor.author | Davies, CL | |
dc.contributor.author | Ennis, J | |
dc.contributor.author | Gardner, T | |
dc.contributor.author | Labdon, A | |
dc.contributor.author | Lanthermann, C | |
dc.contributor.author | Merand, A | |
dc.contributor.author | Rich, E | |
dc.contributor.author | Schaefer, GH | |
dc.contributor.author | Setterholm, BR | |
dc.date.accessioned | 2023-02-06T09:02:24Z | |
dc.date.issued | 2023-04-24 | |
dc.date.updated | 2023-02-05T17:16:56Z | |
dc.description.abstract | Inner regions of protoplanetary disks host many complex physical processes such as star-disk interactions, magnetic fields, planet formation, and the migration of new planets. To directly study this region requires milli-arcsecond angular resolution, beyond the diffraction limit of the world’s largest optical telescopes and even too small for the mm-wave interferometer ALMA. However, we can use infrared interferometers to image the inner astronomical unit. Here, we present new results from the CHARA and VLTI arrays for the young and luminous Herbig Be star HD 190073. We detect a sub-AU cavity surrounded by a ring-like structure that we interpret as the dust destruction front. We model the shape with 6 radial profiles, 3 symmetric and 3 asymmetric, and present a model-free image reconstruction. All the models are consistent with a near face-on disk with inclination . 20◦ , and we measure an average ring radius of 1.35±0.2 mas (1.14 AU). Around 47.6% of the total flux comes from the disk with 15% of that emission appearing to emerge from inside the inner rim. The cause of emission is still unclear, perhaps due to different dust grain compositions or gas emission. The skewed models and the imaging point to an off-center star, possibly due to binarity. Our image shows a sub-AU structure, which seems to move between the two epochs inconsistently with Keplerian motion and we discuss possible explanations for this apparent change. | en_GB |
dc.description.sponsorship | European Research Council (ERC) | en_GB |
dc.description.sponsorship | Science and Technology Facilities Council (STFC) | en_GB |
dc.description.sponsorship | National Science Foundation (NSF) | en_GB |
dc.identifier.citation | Vol. 947 (2), article 68 | en_GB |
dc.identifier.doi | 10.3847/1538-4357/acb4ea | |
dc.identifier.grantnumber | 639889 | en_GB |
dc.identifier.grantnumber | 101003096 | en_GB |
dc.identifier.grantnumber | ST/V000721/1 | en_GB |
dc.identifier.grantnumber | 630008203 | en_GB |
dc.identifier.grantnumber | 1830728 | en_GB |
dc.identifier.uri | http://hdl.handle.net/10871/132421 | |
dc.identifier | ORCID: 0000-0001-6017-8773 (Kraus, Stefan) | |
dc.language.iso | en | en_GB |
dc.publisher | American Astronomical Society / IOP Publishing | en_GB |
dc.rights | © 2023. The Author(s). Published by the American Astronomical Society. Open access. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. | |
dc.title | Imaging the Inner Astronomical Unit of Herbig Be Star HD 190073 | en_GB |
dc.type | Article | en_GB |
dc.date.available | 2023-02-06T09:02:24Z | |
dc.identifier.issn | 0004-637X | |
dc.description | This is the final version. Available on open access from IOP Publishing via the DOI in this record | en_GB |
dc.identifier.journal | Astrophysical Journal | en_GB |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | en_GB |
dcterms.dateAccepted | 2023-01-18 | |
dcterms.dateSubmitted | 2022-08-13 | |
rioxxterms.version | VoR | en_GB |
rioxxterms.licenseref.startdate | 2023-01-18 | |
rioxxterms.type | Journal Article/Review | en_GB |
refterms.dateFCD | 2023-02-05T17:16:58Z | |
refterms.versionFCD | AM | |
refterms.dateFOA | 2023-05-04T14:47:11Z | |
refterms.panel | B | en_GB |
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Except where otherwise noted, this item's licence is described as © 2023. The Author(s). Published by the American Astronomical Society. Open access. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.