Titlebook: Surveys of the Southern Galaxy; Proceedings of a Wor W. B. Burton,F. P. Israel Conference proceedings 1983 Springer Science+Business Media

津贴

Recent 21CM Surveys of the Southern Milky Way and the Distribution of HI Beyond the Solar Circlelayer. The total mass of HI in the Galaxy is found to be 4.8 × 109 M...Time will not permit an overall review of the large-scale structure of atomic hydrogen. Also, the results of the other recent study (by Kulkarni, Blitz, and Heiles) are being discussed separately. This paper will therefore concentrate on the recent work of the Maryland group.

Engaging

The Massachusetts — Stony Brook CO Survey of the Galactic Planeurvey, a two year project to be complete by mid-1983, will provide a map of the entire first quadrant at 3 arc minute spacing, increasing our previous sample by nearly an order of magnitude and allowing an unprecedented view of individual molecular clouds throughout the disk on all size scales between a few parsecs and many kiloparsecs.

子女

Molecular Clouds in the Outer Milky Way Galaxy kinetic temperature in the outer galaxy clouds, and that this had to be taken into account in mass estimates of molecular material in the galaxy. It was estimated that the mass of H. in the outer galaxy is ~ 1/3 that in the inner galaxy.

本土

CO Distribution Along the Southern Galactic Plane≤ 0.075° with an effective angular resolution of about 8′ arc. The variation of radial velocity with longitude shows well-defined terminal velocities whose locus matches closely the rotation curves determined from atomic hydrogen and CO observations along the northern galactic plane. Over particular

Arctic

A First CO(J=2-1) Survey of the Southern Hemispherelumpy; the radial distribution of CO in the fourth quadrant differs from that in the (northern) first quadrant. The cloud-cloud velocity dispersion is, however, very similar to that found in the northern hemisphere.

debase

A Southern Survey of H166α Emission from the Galactic Planens and some preliminary results are presented and discussed. The ionized material along the southern galactic equator exhibits somewhat different longitude and radial distributions than the northern ionized material. Ionized hydrogen in the south is relatively more abundant for R > 6 kpc than in the

织布机

HI Galactic Surveys Done at the IARficas y Técnicas (CONICET), the Comisión de Investigaciones Científicas de la Provincia de Buenos Aires, and the national universities of Buenos Aires and La Plata. The objective was to provide through this Institute the technical and scientific support to install and operate the radiotelescope, for

Defraud

喷油井

亵渎

Gas Content and Gamma Ray Emission in the First Galactic Quadrantactic quadrant and to the high-energy gamma rays (E > 300 MeV). It is found that a simple model, in which uniformly distributed cosmic rays interact with the interstellar gas, can account for the observed gamma-ray emission. Furthermore if the contribution from point sources to the gamma-ray flux is