PRIMARY DISKS AND THEIR OBSERVATIONAL APPEARANCE IN COLLAPSING MAGNETIC ROTATING PROTOSTELLAR CLOUDS
Author:
Publisher
Allerton Press
Subject
Electronic, Optical and Magnetic Materials
Link
https://link.springer.com/content/pdf/10.3103/S1068335621090050.pdf
Reference16 articles.
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2. Andre, Ph., Ward-Thompson, D., and Barsony, M., Submillimeter continuum observations of rho Ophiuchi A: the candidate protostar VLA 1623 and prestellar clumps, Astrophys. J., 1993, vol. 406, p. 122. https://doi.org/10.1086/172425
3. Ohashi, N., Hayashi, M., Ho, P.T.P., and Momose, M., Interferometric imaging of IRAS 04368+2557 in the L1527 molecular cloud core: a dynamically infalling envelope with rotation, Astrophys. J., 1997, vol. 475, pp. 211–223. https://doi.org/10.1086/303533
4. Wiseman, J., Wootten, A., Zinnecker, H., and McCaughrean, M., The flattened, rotating molecular gas core of protostellar jet HH 212, Astrophys. J., 2001, vol. 550, pp. L87–L90. https://doi.org/10.1086/319474
5. Lee, C.-F., Kwon, W., Jhan, K.-S., et al., A pseudodisk threaded with a toroidal and pinched poloidal magnetic field morphology in the HH 211 protostellar system, Astrophys. J., 2019, vol. 879, p. 101. https://doi.org/10.3847/1538-4357/ab2458
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