The Determination of Galactic Arms from the Brightness Distribution of Far Infrared Sources

Author(s):  
Tong Yi ◽  
Sun Jin ◽  
Li Zhong Yuan
1990 ◽  
Vol 139 ◽  
pp. 123-124
Author(s):  
Tong Yi ◽  
Sun Jin ◽  
Li Zhong Yuan

From the IRAS catalogue we selected 10,001 young infrared (IR) sources which lie within the galactic plane. Their IR flux integrated over ±5° in latitude shows maxima at galactic longitudes l = 80°, 60°, 50°, 35°, −27°, −54°, and −74°, which directions are interpreted as tangents to the spiral arms. The resulting spiral arm pattern is nearly identical with the arms derived from observations of O and B stars.


2005 ◽  
Vol 430 (1) ◽  
pp. 343-353 ◽  
Author(s):  
Cs. Kiss ◽  
U. Klaas ◽  
D. Lemke

2017 ◽  
Vol 13 (S336) ◽  
pp. 311-312
Author(s):  
Luca Olmi ◽  
Esteban D. Araya ◽  
Jason Armstrong

AbstractIn 2014 we conducted a survey for 6.7 GHz methanol masers with the Arecibo Telescope toward far infrared sources selected from the Hi-GAL catalog of massive cores. We found a number of sources with weak 6.7 GHz methanol masers, possibly indicating regions in early stages of star formation. Here we describe the results of follow-up observations that were conducted with the Very Large Array in New Mexico to characterize this new population of “weak” 6.7 GHz methanol masers.


2007 ◽  
Vol 667 (1) ◽  
pp. 11-25 ◽  
Author(s):  
N. Odegard ◽  
R. G. Arendt ◽  
E. Dwek ◽  
L. M. Haffner ◽  
M. G. Hauser ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document