Dense gas in the Galactic central molecular zone is warm and heated by turbulence
A&A, 586 (2016) A50
Published online: 2016-01-26
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https://doi.org/10.1093/mnrasl/slw080
Temperature structures in Galactic center clouds
K. Immer, J. Kauffmann, T. Pillai, A. Ginsburg and K. M. MentenAstronomy & Astrophysics 595 A94 (2016)
https://doi.org/10.1051/0004-6361/201628777
A Brief Update on the CMZoom Survey
C. Battersby, E. Keto, Q. Zhang, et al.Proceedings of the International Astronomical Union 11 (S322) 90 (2016)
https://doi.org/10.1017/S1743921316012266
THE LINK BETWEEN TURBULENCE, MAGNETIC FIELDS, FILAMENTS, AND STAR FORMATION IN THE CENTRAL MOLECULAR ZONE CLOUD G0.253+0.016
C. Federrath, J. M. Rathborne, S. N. Longmore, J. M. D. Kruijssen, J. Bally, Y. Contreras, R. M. Crocker, G. Garay, J. M. Jackson, L. Testi and A. J. WalshThe Astrophysical Journal 832 (2) 143 (2016)
https://doi.org/10.3847/0004-637X/832/2/143
How hot is the molecular gas in the Galactic Center?
Katharina Immer, Jens Kauffmann, Thushara Pillai, Adam Ginsburg and Karl M. MentenProceedings of the International Astronomical Union 11 (S322) 111 (2016)
https://doi.org/10.1017/S1743921316012278
The link between solenoidal turbulence and slow star formation in G0.253+0.016
C. Federrath, J. M. Rathborne, S. N. Longmore, et al.Proceedings of the International Astronomical Union 11 (S322) 123 (2016)
https://doi.org/10.1017/S1743921316012357
Positron excess in the center of the Milky Way from short-lived β+ emitting isotopes
M. S. PshirkovPhysical Review D 94 (10) (2016)
https://doi.org/10.1103/PhysRevD.94.103002
High-mass star-forming cloud G0.38+0.04 in the Galactic center dust ridge contains H2CO and SiO masers
Adam Ginsburg, Andrew Walsh, Christian Henkel, et al.Astronomy & Astrophysics 584 L7 (2015)
https://doi.org/10.1051/0004-6361/201527452