The DOI matches its Crossref record; 37 of the 37 references it cites were found in a registry or an index.
A COBE Model of the Galactic Bar and Disk
Open accessAbstract
A model of the bar and old stellar disk of the Galaxy has been derived from the survey of the Diffuse Infrared Background Experiment (DIRBE) of the Cosmic Background Explorer at wavelengths of 1.25, 2.2, 3.5, and 4.9 μm. It agrees very well with the data, except in directions in which the near-infrared optical depth is high. Among the conclusions drawn from the model is that the Sun is located approximately 16.5 pc above the midpoint of the Galactic plane. The disk has an outer edge 4 kpc from the Sun and is warped like the H I layer. It has a central hole roughly the diameter of the inner edge of the 3 kpc molecular cloud ring, and within that hole lies a bright, strong, "early-type" bar, tilted approximately 14° from the Sun-Galactic center line. The model has 47 free parameters. The model is discussed in detail, and contour plots and images of the residuals are presented.
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Cites
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The interstellar extinction law from 1 to 13 microns
Rieke, G. H., & Lebofsky, M. J. (1985) · The Astrophysical Journal · doi:10.1086/162827 · Cited by 2,365
On the Disks of Spiral and so Galaxies
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The existence and shapes of dust lanes in galactic bars
Athanassoula, E. (1992) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/259.2.345 · Cited by 1,011 · cited 1×
“…of other spiral galaxies and with simulations that show that a strong rotating bar sweeps up the gas and dust in its vicinity There seems(Athanassoula 1992b). to be a current consensus that rings form at the inner second harmonic resonance just inside the(Schwartz 1984), corotation…”
BackgroundTHE GALACTIC CENTER ENVIRONMENT
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The universe at faint magnitudes. I - Models for the galaxy and the predicted star counts
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The Distance to the Center of the Galaxy
Reid, M. J., Schneps, M. H., Moran, J. M., Gwinn, C. R., Genzel, R., Downes, D., & Ronnang, B. (1987) · Star Forming Regions · doi:10.1007/978-94-009-4782-5_169 · Cited by 713
A composite CO survey of the entire Milky Way
Dame, T. M., Ungerechts, H., Cohen, R. S., de Geus, E. J., Grenier, I. A., May, J., Murphy, D. C., Nyman, L.-A., & Thaddeus, P. (1987) · The Astrophysical Journal · doi:10.1086/165766 · Cited by 673
Analytical models for galactic nuclei
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Understanding the kinematics of Galactic Centre gas
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Cited by
The Galaxy in Context: Structural, Kinematic, and Integrated Properties
Bland-Hawthorn, J., & Gerhard, O. (2016) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081915-023441 · Cited by 1,656
Abundance Gradients and the Formation of the Milky Way
Chiappini, C., Matteucci, F., & Romano, D. (2001) · The Astrophysical Journal · doi:10.1086/321427 · Cited by 688
Star Formation Thresholds and Galaxy Edges: Why and Where
Schaye, J. (2004) · The Astrophysical Journal · doi:10.1086/421232 · Cited by 615
Licquia, T. C., & Newman, J. A. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/806/1/96 · Cited by 502
Launhardt, R., Zylka, R., & Mezger, P. G. (2002) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20020017 · Cited by 477
Metadata
- Authors
- Freudenreich, H. T.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1998-01-10
- Volume
- 492
- Issue
- 2
- Pages
- 495-510
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1895365318
- Cited by
- 311
- References
- 37
- FWCI
- 9.89
- Type
- journal article
- Language
- en
- Open access
- bronze
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.