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Record W2073021432 · doi:10.1088/0004-637x/762/1/48

SPIRAL ARMS IN THE ASYMMETRICALLY ILLUMINATED DISK OF MWC 758 AND CONSTRAINTS ON GIANT PLANETS

2012· article· en· W2073021432 on OpenAlexaff
C. A. Grady, Takayuki Muto, Jun Hashimoto, Misato Fukagawa, Thayne Currie, Beth Biller, C. Thalmann, Michael L. Sitko, R. W. Russell, John P. Wisniewski, Ruobing Dong, Jungmi Kwon, S. Sai, Jeremy Hornbeck, Glenn Schneider, Dean C. Hines, M. Feldt, Th. Henning, Jörg‐Uwe Pott, M. Bonnefoy, J. Bouwman, S. Lacour, A. Müeller, Á. Juhász, A. Crida, G. Chauvin, Sean M. Andrews, David J. Wilner, Adam L. Kraus, S. E. Dahm, Thomas Robitaille, Hannah Jang‐Condell, L. Abe, Eiji Akiyama, W. Brandner, Timothy D. Brandt, J. Carson, Sebastian Egner, Katherine B. Follette, Miwa Goto, Olivier Guyon, Yutaka Hayano, Masahiko Hayashi, Saeko S. Hayashi, K. W. Hodapp, Miki Ishii, Masanori Iye, M. Janson, Ryo Kandori, G. R. Knapp, Tomoyuki Kudo, Nobuhiko Kusakabe, Masayuki Kuzuhara, Satoshi Mayama, Michael W. McElwain, Taro Matsuo, Shoken M. Miyama, Jun‐Ichi Morino, T. Nishimura, Tae‐Soo Pyo, G. Serabyn, Hiroshi Suto, Ryuji Suzuki, M. Takami, N. Takato, Hiroshi Terada, Daigo Tomono, Edwin L. Turner, Makoto Watanabe, Tōru Yamada, Hideki Takami, Tomonori Usuda, Motohide Tamura

Bibliographic record

VenueThe Astrophysical Journal · 2012
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of Toronto
FundersJapan Society for the Promotion of ScienceNational Aeronautics and Space AdministrationMinistry of Education, Culture, Sports, Science and TechnologySpace Telescope Science InstituteNational Science Foundation
KeywordsPhysicsExoplanetAstrophysicsPlanetDebris diskAstronomyBrown dwarfPlanetary systemAccretion (finance)Spiral (railway)Spiral galaxyStars

Abstract

fetched live from OpenAlex

We present the first near-IR scattered light detection of the transitional disk associated with the Herbig Ae star MWC 758 using data obtained as part of the Strategic Exploration of Exoplanets and Disks with Subaru, and 1.1 μm Hubble Space Telescope /NICMOS data. While submillimeter studies suggested there is a dust-depleted cavity with r = 0 35, we find scattered light as close as 0 1 (20–28 AU) from the star, with no visible cavity at H , K ', or K s . We find two small-scaled spiral structures that asymmetrically shadow the outer disk. We model one of the spirals using spiral density wave theory, and derive a disk aspect ratio of h ∼ 0.18, indicating a dynamically warm disk. If the spiral pattern is excited by a perturber, we estimate its mass to be 5 +3 − 4 M J , in the range where planet filtration models predict accretion continuing onto the star. Using a combination of non-redundant aperture masking data at L ' and angular differential imaging with Locally Optimized Combination of Images at K ' and K s , we exclude stellar or massive brown dwarf companions within 300 mas of the Herbig Ae star, and all but planetary mass companions exterior to 0 5. We reach 5σ contrasts limiting companions to planetary masses, 3–4 M J at 1 0 and 2 M J at 1 55, using the COND models. Collectively, these data strengthen the case for MWC 758 already being a young planetary system.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.016
Threshold uncertainty score0.033

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.013
GPT teacher head0.240
Teacher spread0.227 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations256
Published2012
Admission routes1
Has abstractyes

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