Abstract
An atlas of 21 cm line profiles is described, which was made using a 30 m radio telescope with angular resolution of 0.5 deg, to study the properties of the low latitude H I gas excluding the complexity of the galactic plane. The results of the atlas itself are presented in two sets of diagrams: average profiles for each point, and contour maps. Analyses of the data have centered on an anomalous velocity cloud near galactic longitude (1) equals 349 deg, and latitude (b) equals plus 3 deg, strong kinematic asymmetries of the interstellar gas in the region of 1 between 348 and 12 deg and b between plus 3 and plus 17 deg, with positive radial velocities predominant, caused by a very intense source seemingly identical to Lindblad's (1967) feature A, and a comparative study of optical and radioastronomical data of the section of Gould's belt from 1 equals 300 to 12 deg.
Poeppel, W G.L.;
[1]
Olano, C A
[2]
- Instituto Argentino de Radioastronomia, Villa Elisa, Buenos Aires, Argentina
- Rio Grande do Sul, Universidade Federal, Porto Alegre, Brazil
Citation Formats
Poeppel, W G.L., and Olano, C A.
A low-latitude southern atlas of galactic hydrogen.
Chile: N. p.,
1979.
Web.
Poeppel, W G.L., & Olano, C A.
A low-latitude southern atlas of galactic hydrogen.
Chile.
Poeppel, W G.L., and Olano, C A.
1979.
"A low-latitude southern atlas of galactic hydrogen."
Chile.
@misc{etde_7081623,
title = {A low-latitude southern atlas of galactic hydrogen}
author = {Poeppel, W G.L., and Olano, C A}
abstractNote = {An atlas of 21 cm line profiles is described, which was made using a 30 m radio telescope with angular resolution of 0.5 deg, to study the properties of the low latitude H I gas excluding the complexity of the galactic plane. The results of the atlas itself are presented in two sets of diagrams: average profiles for each point, and contour maps. Analyses of the data have centered on an anomalous velocity cloud near galactic longitude (1) equals 349 deg, and latitude (b) equals plus 3 deg, strong kinematic asymmetries of the interstellar gas in the region of 1 between 348 and 12 deg and b between plus 3 and plus 17 deg, with positive radial velocities predominant, caused by a very intense source seemingly identical to Lindblad's (1967) feature A, and a comparative study of optical and radioastronomical data of the section of Gould's belt from 1 equals 300 to 12 deg.}
journal = []
volume = {3}
journal type = {AC}
place = {Chile}
year = {1979}
month = {Jan}
}
title = {A low-latitude southern atlas of galactic hydrogen}
author = {Poeppel, W G.L., and Olano, C A}
abstractNote = {An atlas of 21 cm line profiles is described, which was made using a 30 m radio telescope with angular resolution of 0.5 deg, to study the properties of the low latitude H I gas excluding the complexity of the galactic plane. The results of the atlas itself are presented in two sets of diagrams: average profiles for each point, and contour maps. Analyses of the data have centered on an anomalous velocity cloud near galactic longitude (1) equals 349 deg, and latitude (b) equals plus 3 deg, strong kinematic asymmetries of the interstellar gas in the region of 1 between 348 and 12 deg and b between plus 3 and plus 17 deg, with positive radial velocities predominant, caused by a very intense source seemingly identical to Lindblad's (1967) feature A, and a comparative study of optical and radioastronomical data of the section of Gould's belt from 1 equals 300 to 12 deg.}
journal = []
volume = {3}
journal type = {AC}
place = {Chile}
year = {1979}
month = {Jan}
}