The Morphology of the Stars, Atomic Gas, and Ionized Gas in the Barred Spiral Galaxy NGC 1530

1996 ◽  
Vol 112 ◽  
pp. 2549 ◽  
Author(s):  
Michael W. Regan ◽  
Peter J. Teuben ◽  
Stuart N. Vogel ◽  
Thijs van der Hulst
1996 ◽  
Vol 157 ◽  
pp. 164-167
Author(s):  
S. N. Dodonov

AbstractIntegral Field Spectrograph observations of southeast (SE) gas outflow in the center (11×13 arcsec) of NGC 4258 with spatial sampling 0.6 and 1.2 arcsec were made with the 6-m Telescope. Reconstructed spatial and kinematic structure of the SE outflow from 20-30 pc to 200-220 pc are presented.


2020 ◽  
Vol 494 (3) ◽  
pp. 4266-4278 ◽  
Author(s):  
G W Roberts-Borsani

ABSTRACT Mass outflow rates and loading factors are typically used to infer the quenching potential of galactic-scale outflows. However, these generally rely on observations of a single gas phase that can severely underestimate the total ejected gas mass. To address this, we use observations of high mass (≥1010 M⊙), normal star-forming galaxies at z ∼ 0 from the MaNGA, xCOLD GASS, xGASS, and ALFALFA surveys and a stacking of Na d, Hα, CO(1–0), and H i 21 cm tracers with the aim of placing constraints on an average, total mass outflow rate, and loading factor. We find detections of outflows in both neutral and ionized gas tracers, with no detections in stacks of molecular or atomic gas emission. Modelling of the outflow components reveals velocities of |vNa d| = 131 km s−1 and |vHα| = 439 km s−1 and outflow rates of $\dot{M}_{\rm {Na\,\small{D}}}$ = 7.55 M⊙ yr−1 and $\dot{M}_{\text{H}\alpha }$ = 0.10 M⊙ yr−1 for neutral and ionized gas, respectively. Assuming a molecular/atomic outflow velocity of 200 km s−1, we derive upper limits of $\dot{M}_{\text{CO}}\lt 19.43$ M⊙ yr−1 and $\dot{M}_{\rm {H\,\small {I}}}\lt $ 26.72 M⊙ yr−1 for the molecular and atomic gas, respectively. Combining the detections and upper limits, we find average total outflow rates of $\dot{M}_{\text{tot}}\lesssim$27 M⊙ yr−1 and a loading factor of ηtot ≲ 6.39, with molecular gas likely contributing ≲72 per cent of the total mass outflow rate, and neutral and ionized gas contributing ∼28 and <1 per cent, respectively. Our results suggest that, to first order, a degree of quenching via ejective feedback could occur in normal galaxies when considering all gas phases, even in the absence of an active galactic nucleus.


1991 ◽  
Vol 101 ◽  
pp. 825 ◽  
Author(s):  
Jean-Rene Roy ◽  
Jianguo Wang ◽  
Robin Arsenault

1978 ◽  
Vol 219 ◽  
pp. 31 ◽  
Author(s):  
C. J. Peterson ◽  
N. Thonnard ◽  
V. C. Rubin ◽  
W. K., Jr. Ford

1985 ◽  
Vol 298 ◽  
pp. 560 ◽  
Author(s):  
W. C. Pence ◽  
G. de Vaucouleurs

1994 ◽  
Vol 431 ◽  
pp. 156 ◽  
Author(s):  
Rene A. M. Walterbos ◽  
Robert Braun
Keyword(s):  

2016 ◽  
Vol 461 (2) ◽  
pp. 1684-1700 ◽  
Author(s):  
Yusuke Fujimoto ◽  
Greg L. Bryan ◽  
Elizabeth J. Tasker ◽  
Asao Habe ◽  
Christine M. Simpson

Sign in / Sign up

Export Citation Format

Share Document