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L1527 IRS

RA (J2000)
DEC (J2000)
Category
SpTy
R band (mag)
Distance (pc)
Disk Diameter (")
Disk Diameter (AU)
Inclination
PADisk
Reference
How Well Resolved
At ref. wavelength (micron)
# References
04 39 53.59 +26 03 05.5YSO1407098009090Tobin et al. 20084.1707
 

Notes:

Extended shadow of edge-on disk

References:

Mustang 3.3 mm Continuum Observations of Class 0 Protostars
Shirley, Y.L. Et al. 2011 A.J. 141 39
 
The Inner Envelope and Disk of L1527 Revealed: Gemini L'-band-scattered Light Imaging
Tobin, J.J., Hartmann, L., Loinard, L. 2010 Ap.J. 722 L12
 
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
 
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
 
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
 
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