The DOI matches its Crossref record; 20 of the 20 references it cites were found in a registry or an index.
The Spitzer/GLIMPSE Surveys: A New View of the Milky Way
Abstract
A brief description is given of the GLIMPSE surveys, including the areas surveyed, sensitivity limits, and products. The primary motivations for this review are to describe some of the main scientific results enabled by the GLIMPSE surveys and to note potential future applications of the GLIMPSE catalogs and images. In particular, we discuss contributions to our understanding of star formation and early evolution, the interstellar medium, galactic structure, and evolved stars. Infrared dark clouds (IRDCs), young stellar objects (YSOs), and infrared bubbles/H II regions are discussed in some detail. A probable triggered star formation associated with expanding infrared bubbles is briefly mentioned. The distribution and morphologies of dust and polycyclic aromatic hydrocarbons (PAHs) in the interstellar medium are discussed. Examples are shown from GLIMPSE images of bow shocks, pillars (elephant trunks), and instabilities in massive star-formation regions. The infrared extinction law of diffuse interstellar dust is discussed. The large-scale structure of the Galaxy has been traced by red-clump giants using the GLIMPSE point-source catalog to reveal the radius and orientation of the central bar, the stellar radial scale length, an obvious increase in star counts toward the tangency to the Scutum-Centaurus spiral arm, the lack of an obvious tangency from star counts toward the Sagittarius spiral arm, and a sharp increase in star counts toward the nuclear bulge. Recent results on evolved stars and some serendipitous discoveries are mentioned. More than 70 refereed papers have been published based on GLIMPSE data as of 2008 November.
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Citations
Cites
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The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 μm Using GLIMPSE Data
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Self-citationDust in the Galactic Environment
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Churchwell, E., Povich, M. S., Allen, D., Taylor, M. G., Meade, M. R., Babler, B. L., Indebetouw, R., Watson, C., Whitney, B. A., Wolfire, M. G., et al. (2006) · The Astrophysical Journal · doi:10.1086/507015 · Cited by 554
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Self-citation
Cited by
Star Formation in the Milky Way and Nearby Galaxies
Kennicutt, R. C., & Evans, N. J. (2012) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081811-125610 · Cited by 2,902
“A conception of what the MW would look like from the outside (Churchwell et al. 2009) is shown in Figure 5.”
BackgroundThe Apache Point Observatory Galactic Evolution Experiment (APOGEE)
Majewski, S. R., Schiavon, R. P., Frinchaboy, P. M., Prieto, C. A., Barkhouser, R., Bizyaev, D., Blank, B., Brunner, S., Burton, A., Carrera, R., et al. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa784d · Cited by 1,831
Trigonometric Parallaxes of High-mass Star-forming Regions: Our View of the Milky Way
Reid, M. J., Menten, K. M., Brunthaler, A., Zheng, X. W., Dame, T. M., Xu, Y., Li, J., Sakai, N., Wu, Y., Immer, K., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab4a11 · Cited by 760
THE MILKY WAY'S CIRCULAR-VELOCITY CURVE BETWEEN 4 AND 14 kpc FROM APOGEE DATA
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Pecaut, M. J., & Mamajek, E. E. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1300 · Cited by 407
Metadata
- Authors
- Churchwell, E., Babler, B. L., Meade, M. R., Whitney, B. A., Benjamin, R., Indebetouw, R., Cyganowski, C., Robitaille, T. P., Povich, M., Watson, C., & Bracker, S.
- Venue
- Publications of the Astronomical Society of the Pacific
- Publisher
- IOP Publishing
- Published
- 2009-03
- Volume
- 121
- Issue
- 877
- Pages
- 213-230
- ISSN
- 0004-6280 (ISSN-L)
- 1538-3873
- OpenAlex
- W2259968672
- Cited by
- 1,047
- References
- 20
- FWCI
- 26.56
- Type
- journal article
- Language
- en
- Open access
- closed
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