SFChem 2002: Chemistry as a Diagnostic of Star Formation
By C. Curry, M. Fich. 2003
143 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/59204bfd35428bbd03f1fff32e942fe50f4cecd6
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- Imaging the Disk around TW Hydrae with the Submillimeter Array (2004, background): “The prospects are excellent for interferometric observations of protoplanetary disks at submillimeter wavelengths (Blake 2003).”
- Organic molecules in protoplanetary disks around T Tauri and Herbig Ae stars (2004, background): “Searches for other deuterated species in the LkCa 15 disk, in particular DCN and HDO, are reported by Kessler et al. (2003).”
- Probing the Evolutionary Status of Starless Cores through N2H+ and N2D+ Observations (2004, unknown): “In particular, looking at the density peak, we expect a ‘‘blue shoulder’’ in the case of outflow motions and a ‘‘red shoulder’’ in the case of infall motions (for a review see Evans 2002).”
- The initial conditions of isolated star formation — VI. SCUBA mapping of pre-stellar cores (2005, methodology): “Furthermore, for one of the cores, L1689B, they use a value for the inter-stellar radiation field (ISRF) that is too small for the environs of Ophiuchus in which L1689B is situated (c.f. André et al. 2003).”
- The Mid-Infrared Instrument for the James Webb Space Telescope, VI: The Medium Resolution Spectrometer (2015, methodology): “For the initial analysis, we follow the formalism as defined in Kester et al. (2003) and Lahuis & Boogert (2003).”
- The initial conditions of star formation in the Ophiuchus main cloud: Kinematics of the protocluster condensations , (2007, unknown): “Our adopted defaultTd = 12 K is consistent with the typical mass-averaged temperature found by dust radiative transfer models of starless cores (cf. André et al. 2003; Stamatellos & Whitworth 2003).”
- Far-infrared to millimeter astrophysical dust emission. I. A model based on physical properties of a (2007, background): “Key words. dust, extinction – diffuse radiation – infrared: ISM – radio continuum: ISM – scattering – radiation mechanisms: thermal”