[SZH2010] W51e2-W , the SIMBAD biblio

[SZH2010] W51e2-W , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST08:54:27

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2010ApJ...710..843S 1487     A D S   X C       38 18 26 Nature of W51e2: massive cores at different phases of star formation. SHI H., ZHAO J.-H. and HAN J.L.
2010ApJ...718L.181S 710     A     X C       18 7 18 A bipolar outflow from the massive protostellar core W51e2-E. SHI H., ZHAO J.-H. and HAN J.L.
2010ApJ...720.1055S viz 40           X         1 28 149 Trigonometric parallax of W51 Main/South. SATO M., REID M.J., BRUNTHALER A., et al.
2012MNRAS.423..647E 155           X         4 19 19 Methanol and excited OH masers towards W51 – I. Main and south. ETOKA S., GRAY M.D. and FULLER G.A.
2011PASP..123..516S 5 0 Cores and outflows of star formation region W51e2 and highly polarized radio sources in the NVSS. (Dissertation summary). SHI H.
2016A&A...589A..44G viz 1188     A S   X         29 17 4 Hot ammonia around young O-type stars. III. High-mass star formation and hot core activity in W51 Main. GODDI C., GINSBURG A. and ZHANG Q.
2016A&A...595A..27G viz 41           X         1 29 54 Toward gas exhaustion in the W51 high-mass protoclusters. GINSBURG A., GOSS W.M., GODDI C., et al.
2018ApJ...855...39K 593       D     X C       14 22 15 Polarization properties and magnetic field structures in the high-mass star-forming region W51 observed with ALMA. KOCH P.M., TANG Y.-W., HO P.T.P., et al.
2022ApJ...932....5K 90           X         2 19 1 Spectral-line Survey of the Region of Massive Star Formation W51e1/e2 in the 4 mm Wavelength Range. KALENSKII S.V., KAISER R.I., BERGMAN P., et al.
2022ApJ...940...89K 941           X C       20 28 ~ A Multiscale Picture of the Magnetic Field and Gravity from a Large-scale Filamentary Envelope to Core-accreting Dust Lanes in the High-mass Star-forming Region W51. KOCH P.M., TANG Y.-W., HO P.T.P., et al.

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