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SIMBA survey of southern high-mass star forming regions: I. Physical parameters of the $\mathsf{1.2}$-mm/IRAS sources
Open accessAbstract
We report the results of a 1.2 mm continuum emission survey toward 146 IRAS sources thought to harbour high-mass star forming regions. The sources have FIR colors typical of UCHII regions and were detected in the CS() line survey of Bronfman et al. ([CITE]). Regions of , centered on each IRAS source, were mapped with an angular resolution of ~24´´, using the SIMBA array on the SEST telescope. 1.2 mm emission was detected toward all IRAS sources. We find that the dust cores associated with these sources have typical sizes of 0.4 pc and masses of . Dust temperatures and luminosities, derived from the SED, are typically 32 K and .
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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
“Very similar results were obtained from studies of millimeter continuum emission from dust (Faúndez et al. 2004) toward a sample of southern hemisphere sources surveyed in CS J = 2 → 1 (Bronfman et al. 1996).”
ResultKrumholz, M. R. (2014) · Physics Reports · doi:10.1016/j.physrep.2014.02.001 · Cited by 321
Metadata
- Authors
- Faúndez, S., Bronfman, L., Garay, G., Chini, R., Nyman, L.-Å., & May, J.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2004-10
- Volume
- 426
- Issue
- 1
- Pages
- 97-103
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2109771736
- Cited by
- 249
- References
- 0
- FWCI
- 8.86
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: SIMBA survey of southern high-mass star forming regions: I. Physical parameters of the $\mathsf{1.2}$-mm/IRAS sources. https://app.cochat.ai/papers/10.1051/0004-6361:20035755
- The paper
- Faúndez, S., Bronfman, L., Garay, G., Chini, R., Nyman, L.-Å., & May, J. (2004). SIMBA survey of southern high-mass star forming regions: I. Physical parameters of the $\mathsf{1.2}$-mm/IRAS sources. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20035755
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