[TOS2014] MMS-3 , the SIMBAD biblio

[TOS2014] MMS-3 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST20:00:48


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Title First 3 Authors
2014ApJ...789L...4T 135       D     X         4 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 78           X         2 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 212       D     X         6 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...839...69M 81           X         2 10 47 Circumstellar disks and outflows In turbulent molecular cloud cores: possible formation mechanism for misaligned systems. MATSUMOTO T., MACHIDA M.N. and INUTSUKA S.-I.
2017ApJ...849..101T 40           X         1 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 258       D     X         7 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.
2020A&A...635A.189F 412           X C       9 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.
2023PASJ...75..120F 218           X         5 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.
2024ApJ...965...99T 90           X         2 9 ~ Discovery of Asymmetric Spike-like Structures of the 10 au Disk around the Very Low-luminosity Protostar Embedded in the Taurus Dense Core MC 27/L1521F with ALMA. TOKUDA K., HARADA N., OMURA M., et al.

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