Constraining the Envelope Structure of L1527 IRS: Infrared Scattered Light Modeling
*Tobin, J. J., Hartmann, L., Calvet, N., D'Alessio, P., 2008, ApJ, 679, 1364
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Spitzer IRS Spectra and Envelope Models of Class I Protostars in Taurus
Furlan, E., McClure, M., Calvet, N., Hartmann, L., D'Alessio, P., Forrest, W. J., Watson, D. M., Uchida, K. I., Sargent, B., Green, J. D., Herter, T. L., 2008, ApJ, 176, 184
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Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting Observed SEDs Using a Large Grid of Precomputed Models
Robitaille, T. P., Whitney, B. A., Indebetouw, R., Wood, K., 2007, ApJ, 169, 328
| Referred to as IRAS 04368+2557 | |
Tracing the Mass during Low-Mass Star Formation. III. Models of the Submillimeter Dust Continuum Emission from Class 0 Protostars
Shirley, Y.L., Evans, N.J., II, Rawlings, J. M. C., 2002, ApJ, 575, 337
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Interferometric Imaging of IRAS 04368+2557 in the L1527 Molecular Cloud Core: A Dynamically Infalling Envelope with Rotation
Ohashi, N., Hayashi, M., Ho, P. T. P., Momose, M., 1997, ApJ, 475, 211
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