MétaCan
Menu
← Back to cohort
Record W2015737155 · doi:10.1086/340561

Nobeyama Millimeter Array CO (<i>J</i> = 1–0) Observations of the Hα/Radio Lobe Galaxy NGC 3079: Gas Dynamics in a Weak Bar Potential and Central Massive Core

2002· article· en· W2015737155 on OpenAlexaff
Jin Koda, Yoshiaki Sofue, Kotaro Kohno, H. Nakanishi, Shin‐ichi Onodera, S. K. Okumura, J. Irwin

Bibliographic record

VenueThe Astrophysical Journal · 2002
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsQueen's University
Fundersnot available
KeywordsPhysicsAstrophysicsRADIUSSpiral galaxyMillimeterGalaxyBar (unit)Spiral (railway)Submillimeter ArrayCore (optical fiber)AstronomyStar formationOptics

Abstract

fetched live from OpenAlex

We present 12 CO (1-0) observations in the central 4.5 kpc (1') of the Hα/radio lobe galaxy NGC 3079 with the Nobeyama Millimeter Array. The molecular gas shows four components: a main disk, spiral arms, a nuclear disk, and a nuclear core. The main disk extends along the galaxy major axis. We detected its central 2 kpc radius, while its full extent is beyond our spatial coverage. Molecular gas is smoothly distributed in the main disk, having a gas mass of 5 × 10 9 M ☉ within the central ~2 kpc radius. The spiral arms are superimposed on the main disk. Abrupt velocity changes of up to ~200 km s -1 are observed along the spiral arms in S-shaped twists of isovelocity contours and double velocity-peaked features on the spectra. The nuclear disk with ~600 pc radius appears in position-velocity (PV) diagrams, having an intense concentration of molecular gas. Its appearance on PV diagrams is indicative of oval motions of the gas, rather than circular. The nuclear disk and spiral arms form the so-called figure-of-eight pattern on a PV diagram. The nuclear core is more compact than our current resolution (2'' = 150 pc) and has a gas mass of 3 × 10 8 M ☉ within the central 150 pc. Although it is unresolved, the nuclear core shows a very high velocity ~200 km s -1 even at the radius of ~100 pc on the PV diagram. We propose a model that NGC 3079 contains a weak bar. The weak bar model explains the observed features of the main disk, spiral arms, and nuclear disk. The main disk and spiral arms result from gaseous x 1 -orbits and associated crowding, respectively. The nuclear disk arises from gaseous x 2 -orbits. The gas concentration in the nuclear disk could be explained by the expected gas-fueling mechanism: the gas on x 1 -orbits flows along spiral arms (or offset shocks), colliding with the gas on x 2 -orbits, and accumulating onto the nuclear disk. Assuming that the gas moves nearly along the spiral arms that run perpendicular to the line of sight, the pattern speed of the bar is estimated to be 55 ± 10 km s -1 kpc -1 . The high velocity of the nuclear core cannot be explained by our model for a bar. Thus we attribute it to a central massive core with a dynamical mass of 10 9 M ☉ within the central 100 pc. This mass is 3 orders of magnitude more massive than that of a central black hole in this galaxy.

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 score0.005
Threshold uncertainty score0.011

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.001

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 head0.010
GPT teacher head0.194
Teacher spread0.184 · 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

Citations58
Published2002
Admission routes1
Has abstractyes

Explore more

Same venueThe Astrophysical Journal→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→