[TTK2018] Per-emb-33-C , the SIMBAD biblio

[TTK2018] Per-emb-33-C , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST22:14:19


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Title First 3 Authors
2016Natur.538..483T 22 8 183 A triple protostar system formed via fragmentation of a gravitationally unstable disk. TOBIN J.J., KRATTER K.M., PERSSON M.V., et al.
2017MNRAS.469.3881S viz 16       D               1 86 19 Embedded binaries and their dense cores. SADAVOY S.I. and STAHLER S.W.
2018ApJ...852...18T 140       D     X         4 44 10 The VLA Nascent Disk and Multiplicity survey of Perseus protostars (VANDAM). III. Extended radio emission from protostars in Perseus. TYCHONIEC L., TOBIN J.J., KARSKA A., et al.
2019A&A...621A..76M 85           X         2 80 90 Characterizing young protostellar disks with the CALYPSO IRAM-PdBI survey: large Class 0 disks are rare. MAURY A.J., ANDRE P., TESTI L., et al.
2020A&A...635A..15M 44           X         1 37 42 Searching for kinematic evidence of Keplerian disks around Class 0 protostars with CALYPSO. MARET S., MAURY A.J., BELLOCHE A., et al.
2021ApJ...907L..10R 2656     A D S   X C       60 12 15 Kinematic analysis of a protostellar multiple system: measuring the protostar masses and assessing gravitational instability in the disks of L1448 IRS3B and L1448 IRS3A. REYNOLDS N.K., TOBIN J.J., SHEEHAN P., et al.
2021ApJ...910...20Y 17       D               4 85 52 The Perseus ALMA Chemistry Survey (PEACHES). I. The complex organic molecules in Perseus embedded protostars. YANG Y.-L., SAKAI N., ZHANG Y., et al.
2021A&A...648A..45P 366       D     X         9 65 24 The CALYPSO IRAM-PdBI survey of jets from Class 0 protostars. Exploring whether jets are ubiquitous in young stars. PODIO L., TABONE B., CODELLA C., et al.
2022ApJ...930...67G 63       D     X C       1 39 3 Effects of Magnetic Field Orientations in Dense Cores on Gas Kinematics in Protostellar Envelopes. GUPTA A., YEN H.-W., KOCH P., et al.
2024ApJ...963..164R 270       D     X         6 50 ~ The Disk Orientations of Perseus Protostellar Multiples at ∼8 au Resolution. REYNOLDS N.K., TOBIN J.J., SHEEHAN P.D., et al.

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