GAL 000.340+00.055 , the SIMBAD biblio

GAL 000.340+00.055 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST04:57:37


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Keywords
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Title First 3 Authors
2012A&A...548A.120I 76               F     1 24 45 A multi-wavelength view of the Galactic Center dust ridge reveals little star formation. IMMER K., MENTEN K.M., SCHULLER F., et al.
2015MNRAS.449..715W 79               F     1 15 45 Tracing the conversion of gas into stars in Young Massive Cluster Progenitors. WALKER D.L., LONGMORE S.N., BASTIAN N., et al.
2018MNRAS.474.2373W 297       D     X C F     6 26 15 Star formation in a high-pressure environment: an SMA view of the Galactic Centre dust ridge. WALKER D.L., LONGMORE S.N., ZHANG Q., et al.
2024ApJ...962...39L 90     A D     X C       2 19 ~ Magnetic Fields in the Central Molecular Zone Influenced by Feedback and Weakly Correlated with Star Formation. LU X., LIU J., PILLAI T., et al.
2025ApJ...978...28P 439       D S   X C       8 15 ~ SOFIA/HAWC+ Far-infrared Polarimetric Large-area CMZ Exploration Survey. IV. Relative Magnetic Field Orientation throughout the CMZ. PARE D.M., CHUSS D.T., KARPOVICH K., et al.
2025ApJ...982L..22K 93             C       1 13 ~ The JCMT BISTRO Survey: Magnetic Fields Align with Orbital Structure in the Galactic Center. KAROLY J., WARD-THOMPSON D., PATTLE K., et al.
2025ApJ...984..157B 112       D     X         3 17 ~ 3D CMZ. II. Hierarchical Structure Analysis of the Central Molecular Zone. BATTERSBY C., WALKER D.L., BARNES A., et al.
2025ApJ...984..159L 19       D               1 14 ~ 3D CMZ. IV. Distinguishing Near versus Far Distances in the Galactic Center Using Spitzer and Herschel. LIPMAN D., BATTERSBY C., WALKER D.L., et al.
2025PASJ...77..687S 47           X         1 19 ~ The Galactic Center arms inferred from the ALMA CMZ Exploration Survey (ACES). SOFUE Y., OKA T., LONGMORE S.N., et al.
2025ApJ...991..156P 93           X         2 12 ~ Parallel Alignments between Magnetic Fields and Dense Structures in the Central Molecular Zone. PAN X., ZHANG Q., QIU K., et al.

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