SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment
| hal.structure.identifier | Department of Astronomy [Ithaca] | |
| dc.contributor.author | ADAMS, J. D., | |
| hal.structure.identifier | Department of Astronomy [Ithaca] | |
| dc.contributor.author | HERTER, T. L., | |
| dc.contributor.author | HORA, J. L., | |
| hal.structure.identifier | KOSMA, I. Physikalisches Institut | |
| dc.contributor.author | SCHNEIDER, N. | |
| hal.structure.identifier | City University of Hong Kong [Hong Kong] [CUHK] | |
| dc.contributor.author | LAU, R. M., | |
| dc.contributor.author | STAUGHN, J. G., | |
| dc.contributor.author | SIMON, R., | |
| hal.structure.identifier | Department of Epidemiology, University of Washington | |
| hal.structure.identifier | Seattle Epidemiologic Research and Information Center of the Department of Veterans Affairs Office of Research and Development | |
| dc.contributor.author | SMITH, N., | |
| dc.contributor.author | GEHRZ, R. D., | |
| dc.contributor.author | ALLEN, L. E., | |
| hal.structure.identifier | FORMATION STELLAIRE 2015 | |
| dc.contributor.author | BONTEMPS, Sylvain | |
| dc.contributor.author | CAREY, S. J., | |
| hal.structure.identifier | USDA, Plant Genet Resources Unit | |
| dc.contributor.author | FAZIO, G. G., | |
| dc.contributor.author | GUTERMUTH, R. A., | |
| dc.contributor.author | GUZMAN FERNANDEZ, A., | |
| hal.structure.identifier | General Practice | |
| dc.contributor.author | HANKINS, M., | |
| hal.structure.identifier | Joint ALMA Observatory [JAO] | |
| dc.contributor.author | HILL, T., | |
| dc.contributor.author | KETO, E., | |
| dc.contributor.author | KOENIG, X. P., | |
| dc.contributor.author | KRAEMER, K. E., | |
| dc.contributor.author | MEGEATH, S. T., | |
| dc.contributor.author | MIZUNO, D. R., | |
| hal.structure.identifier | Procédés, Matériaux et Energie Solaire [PROMES] | |
| dc.contributor.author | MOTTE, F., | |
| dc.contributor.author | MYERS, P. C., | |
| hal.structure.identifier | Miami University [Ohio] [MU] | |
| dc.contributor.author | SMITH, H. A., | |
| dc.date.issued | 2015-10 | |
| dc.identifier.issn | 0004-637X | |
| dc.description.abstractEn | We present mid-IR (19 - 37 microns) imaging observations of S106 from SOFIA/FORCAST, complemented with IR observations from Spitzer/IRAC (3.6 - 8.0 microns), IRTF/MIRLIN (11.3 and 12.5 microns), and Herschel/PACS (70 and 160 microns). We use these observations, observations in the literature, and radiation transfer modeling to study the heating and composition of the warm (~ 100 K) dust in the region. The dust is heated radiatively by the source S106 IR, with little contributions from grain-electron collisions and Ly-alpha radiation. The dust luminosity is >~ (9.02 +/- 1.01) x 10^4 L_sun, consistent with heating by a mid- to late-type O star. We find a temperature gradient (~ 75 - 107 K) in the lobes, which is consistent with a dusty equatorial geometry around S106 IR. Furthermore, the SOFIA observations resolve several cool (~ 65 - 70 K) lanes and pockets of warmer (~ 75 - 90 K) dust in the ionization shadow, indicating that the environment is fragmented. We model the dust mass as a composition of amorphous silicates, amorphous carbon, big grains, very small grains, and PAHs. We present the relative abundances of each grain component for several locations in S106. | |
| dc.language.iso | en | |
| dc.publisher | American Astronomical Society | |
| dc.subject.en | Astrophysics - Solar and Stellar Astrophysics | |
| dc.title.en | SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment | |
| dc.type | Article de revue | |
| dc.identifier.doi | 10.1088/0004-637X/814/1/54 | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA] | |
| dc.identifier.arxiv | 1510.04360 | |
| bordeaux.journal | The Astrophysical Journal | |
| bordeaux.page | id. 54 | |
| bordeaux.volume | 814 | |
| bordeaux.issue | 1 | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-01217944 | |
| hal.version | 1 | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-01217944v1 | |
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