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ALMA Imaging of a Galactic Molecular Outflow in NGC4945
Alberto D. Bolatto, Adam K. Leroy, Rebecca C. Levy +10
We present the ALMA detection of molecular outflowing gas in the central regions of NGC4945, one of the nearest starbursts and also one of the nearest hosts of an active galactic n…
The EDGE-CALIFA survey: The resolved star formation efficiency and local physical conditions
V. Villanueva, A. Bolatto, S. Vogel +14
We measure the star formation rate (SFR) per unit gas mass and the star formation efficiency (SFE for total gas, SFE for the molecular gas) in 81 nearby gal…
Clustered Star Formation in the center of NGC 253 Contributes to Driving the Ionized Nuclear Wind
E. A. C. Mills, M. Gorski, K. L. Emig +12
We present new 3 mm observations of the ionized gas toward the nuclear starburst in the nearby (D ~ 3.5 Mpc) galaxy NGC 253. With ALMA, we detect emission from the H40-alpha and He…
NOEMA High Fidelity Imaging of the Molecular Gas in and around M82
Nico Krieger, Fabian Walter, Alberto D. Bolatto +11
We present a 154 pointing IRAM NOEMA mosaic of the CO(1-0) line emission in and around the nearby starburst galaxy M82. The observations, complemented by zero--spacing observations…
Characterizing the Multi-Phase Origin of [CII] Emission in M101 and NGC 6946 with Velocity Resolved Spectroscopy
Elizabeth Tarantino, Alberto D. Bolatto, Rodrigo Herrera-Camus +10
The [CII] fine-structure transition at 158 micron is frequently the brightest far-infrared line in galaxies. Due to its low ionization potential, C+ can trace the ionized, atomic,…
The EDGE-CALIFA survey: The local and global relations between , and that regulate star-formation
S. F. Sánchez, J. K. Barrera-Ballesteros, D. Colombo +9
We present a new characterization of the relations between star-formation rate, stellar mass and molecular gas mass surface densities at different spatial scales across galaxies (f…
EDGE-CALIFA survey: Self-regulation of Star formation at kpc scales
J. K. Barrera-Ballesteros, S. F. Sánchez, T. Heckman +11
We present the relation between the star formation rate surface density, , and the hydrostatic mid-plane pressure, P, for 4260 star-forming regions of kpc si…