JCMTSF J174621.0-285001 , the SIMBAD biblio

JCMTSF J174621.0-285001 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:21:01


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Title First 3 Authors
1987AJ.....94.1178Y 5 5 144 G 0.18-0.04 : interaction of thermal and nonthermal radio structures in the Arc near the Galactic Center. YUSEF-ZADEH F. and MORRIS M.
1997ApJ...474..275L 15 34 VLA H92α and H115β recombination line observations of the Galactic center H II regions: the Sickle (G0.18-0.04) and the Pistol (G0.15-0.05). LANG C.C., GOSS W.M. and WOOD D.O.S.
2008ApJS..175..277D viz 15       D               7164 308 The SCUBA legacy catalogues: submillimeter-continuum objects detected by SCUBA. DI FRANCESCO J., JOHNSTONE D., KIRK H., et al.
2011PASJ...63..763T 38           X         1 20 33 Sagittarius A Molecular Cloud Complex in H13CO+ and thermal SiO emission lines. TSUBOI M., TADAKI K., MIYAZAKI K., et al.
2016ApJ...826..218L 9386 T   A S   X C       236 10 4 The unusual Galactic Center radio source
N3.
LUDOVICI D.A., LANG C.C., MORRIS M.R., et al.
2018ApJ...852...11B 321           X         8 15 6 M0.20-0.033: an expanding molecular shell in the Galactic Center Radio Arc. BUTTERFIELD N., LANG C.C., MORRIS M., et al.
2019ApJ...884..170P 122           X         3 19 ~ A VLA polarimetric study of the Galactic Center Radio Arc: characterizing polarization, rotation measure, and magnetic field properties. PARE D.M., LANG C.C., MORRIS M.R., et al.
2019ApJ...885...72S 1032       D     X C       25 23 ~ 2 mm GISMO observations of the Galactic Center. II. A nonthermal filament in the Radio Arc and compact sources. STAGUHN J., ARENDT R.G., DWEK E., et al.
2020ApJ...889..174B 2577 T   A S   X C       60 10 ~ 6.7 GHz CH3OH absorption toward the
N3 Galactic Center point source.
BUTTERFIELD N.O., GINSBURG A., LUDOVICI D.A., et al.
2022A&A...664A..49G 170           X         4 35 3 Radio observations of massive stars in the Galactic centre: The Quintuplet cluster. GALLEGO-CALVENTE A.T., SCHODEL R., ALBERDI A., et al.
2025A&A...700A.246C 140           X         3 50 ~ A multi-frequency, multi-epoch radio continuum study of the Quintuplet cluster with the Very Large Array. CANO-GONZALEZ M., SCHODEL R., ALBERDI A., et al.

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