scholarly journals The role of PAHs in the physics of the interstellar medium

2011 ◽  
Vol 46 ◽  
pp. 415-426 ◽  
Author(s):  
L. Verstraete
Keyword(s):  
2020 ◽  
Vol 891 (2) ◽  
pp. 157 ◽  
Author(s):  
Evan Heintz ◽  
Chad Bustard ◽  
Ellen G. Zweibel
Keyword(s):  

2000 ◽  
Vol 197 ◽  
pp. 161-174
Author(s):  
Gary J. Melnick

The Submillimeter Wave Astronomy Satellite (SWAS) was successfully launched on 5 December 1998 with the goals of studying: (1) the distribution of oxygen in the interstellar medium; (2) the role of H2O and O2 as gas coolants; and (3) the UV-illuminated surfaces of molecular clouds. To achieve these goals, SWAS is conducting pointed observations of dense (n(H2) > 103 cm–3) molecular clouds throughout our Galaxy in either the ground-state or a low-lying transition of five astrophysically important species: H2O, H218O, O2, CI, and 13CO. SWAS has made great strides in each of these areas of investigation. This paper will summarize our H2O and O2 findings one year into the mission.


1980 ◽  
Vol 87 ◽  
pp. 411-416
Author(s):  
W.H. Mccutcheon ◽  
R. L. Dickman ◽  
W.L.H. Shuter ◽  
R. S. Roger

Since 13C is believed to be produced by non-equilibrium CNO processing in stellar evolution (Truran 1977), measurements of the carbon ratio Rc ≡ [12C] / [13C] in the interstellar medium may provide important information on nucleo-synthesis. Commonly, the ratio (N13/N18)LTE ≡ [13CO/C18O]LTE is measured and from this RLTE ≡ [12CO/13CO]LTE is deduced and these values are often identified with Rc. However, this line of reasoning can be misleading for two reasons (Dickman et al. 1979):(1) The difficulty of determining accurate column densities, [13C16O] and [12C18O], because of the complexity of the radiative transfer problem;(2) The possible role of fractionation, whereby RCO ≡ [12CO] / [13CO] does not necessarily reflect the initial atomic abundance ratio RC (Watson et al. 1976, Langer 1977, Liszt 1978).


2003 ◽  
Vol 209 ◽  
pp. 525-526 ◽  
Author(s):  
F. Kerber ◽  
F. Guglielmetti ◽  
R. Mignani ◽  
M. Roth

Using Hα images from the Southern H-Alpha Sky Survey Atlas (SHASSA) we have discovered a “cometary tail” of ionized matter extending at least 30 arcmin from the main body of the planetary nebula Sh 2-68 (PN G030.6+06.2). This tail is aligned with the proper motion of the central star and is obviously a contrail of material left behind by Sh 2-68 moving in a Galactic Disk orbit. The tail's existence is a direct confirmation of Sh 2-68's interaction with the interstellar medium (ISM) and highlights the possibly important role of the ISM's magnetic field.


2013 ◽  
Vol 65 (3) ◽  
pp. 213-222 ◽  
Author(s):  
Ryosuke S. Asano ◽  
Tsutomu T. Takeuchi ◽  
Hiroyuki Hirashita ◽  
Akio K. Inoue

2014 ◽  
Vol 441 (1) ◽  
pp. 525-531 ◽  
Author(s):  
A. P. Walker ◽  
B. K. Gibson ◽  
K. Pilkington ◽  
C. B. Brook ◽  
P. Dutta ◽  
...  
Keyword(s):  

2009 ◽  
Vol 146 (1-4) ◽  
pp. 295-327 ◽  
Author(s):  
G. P. Zank ◽  
N. V. Pogorelov ◽  
J. Heerikhuisen ◽  
H. Washimi ◽  
V. Florinski ◽  
...  

2010 ◽  
Vol 712 (1) ◽  
pp. 536-557 ◽  
Author(s):  
Amanda A. Kepley ◽  
Stefanie Mühle ◽  
John Everett ◽  
Ellen G. Zweibel ◽  
Eric M. Wilcots ◽  
...  

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