[TOS2014] MMS-1 , the SIMBAD biblio

[TOS2014] MMS-1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST06:44:01


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Title First 3 Authors
2014ApJ...789L...4T 97       D     X         3 7 47 ALMA observations of a high-density core in Taurus: dynamical gas interaction at the possible site of a multiple star formation. TOKUDA K., ONISHI T., SAIGO K., et al.
2015MNRAS.449L.123M 40           X         1 9 13 An origin of arc structures deeply embedded in dense molecular cloud cores. MATSUMOTO T., ONISHI T., TOKUDA K., et al.
2016ApJ...826...26T 523     A D     X         14 14 16 Revealing a detailed mass distribution of a high-density core MC27/L1521F in Taurus with ALMA. TOKUDA K., ONISHI T., MATSUMOTO T., et al.
2017ApJ...849..101T 975       S   X C       22 9 8 A detached protostellar disk around a ∼0.2 M protostar in a possible site of a multiple star formation in a dynamical environment in Taurus. TOKUDA K., ONISHI T., SAIGO K., et al.
2018ApJ...862....8T 429       D     X C       10 9 11 Warm CO gas generated by possible turbulent shocks in a low-mass star-forming dense core in Taurus. TOKUDA K., ONISHI T., SAIGO K., et al.
2019A&A...628A.112K 47           X         1 8 41 The bridge: a transient phenomenon of forming stellar multiples. Sequential formation of stellar companions in filaments around young protostars. KUFFMEIER M., CALCUTT H. and KRISTENSEN L.E.
2019ApJ...887..209A 42           X         1 32 ~ Protostellar evolution in Serpens Main: possible origin of disk-size diversity. ASO Y., HIRANO N., AIKAWA Y., et al.
2020A&A...635A.189F 639           X C       14 11 ~ Seeds of Life in Space (SOLIS). VII. Discovery of a cold dense methanol blob toward the L1521F VeLLO system. FAVRE C., VASTEL C., JIMENEZ-SERRA I., et al.
2020A&A...637A..92G 44           X         1 31 41 Angular momentum profiles of Class 0 protostellar envelopes. GAUDEL M., MAURY A.J., BELLOCHE A., et al.
2023PASJ...75..120F 280           X         6 5 ~ Twisted magnetic field in star formation processes of L1521 F revealed by submillimeter dual-band polarimetry using the James Clerk Maxwell Telescope. FUKAYA S., SHINNAGA H., FURUYA R.S., et al.

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