Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Harold F. Weaver"'
Publikováno v:
2018 Joint Propulsion Conference.
Publikováno v:
Cryogenics. 52:296-300
The National Aeronautics and Space Administration (NASA) Glenn Research Center (GRC) Plum Brook Station (PBS) Space Propulsion Research Facility, commonly referred to as B-2, is NASA s third largest thermal vacuum facility. It is the largest designed
Publikováno v:
AIP Conference Proceedings.
The National Aeronautics and Space Administration (NASA) Glenn Research Center (GRC) Plum Brook Station (PBS) Spacecraft Propulsion Research Facility, commonly referred to as B-2, is NASA's third largest thermal vacuum facility. It is the largest des
Autor:
Harold F. Weaver
Publikováno v:
Symposium - International Astronomical Union. 84:295-300
The distribution of the column density of HI over the sky shows strongly organized features of large angular extent. In particular, there is (1) a conspicuous set of arching concentric filaments extending more than 80° on either side of ℓ = 330°,
Autor:
Harold F. Weaver
Publikováno v:
Symposium - International Astronomical Union. 39:22-50
The task assigned for this review is to discuss structural features of the Galaxy as they may involve or relate to gas dynamics. Since a topic of such great breadth would permit discussion of essentially any aspect of the Galaxy, we shall narrow the
Autor:
Harold F. Weaver
Publikováno v:
Vistas in Astronomy. 1:228-238
The large K term associated with bright early B stars signifies expansion, but does not indicate any fundamental characteristic of the local region of the galaxy. It is a change property of the sample population traceable to nearby community motion g
Autor:
Harold F. Weaver
Publikováno v:
Symposium - International Astronomical Union. 20:92-99
I. Expansion of the Gaseous and Stellar Components of the GalaxyIf the gaseous component of the Galaxy is expanding as observed by Rougoor and Oort in the centre of the Galaxy and as postulated by Kerr in his early interpretation of spiral structure,
Autor:
Harold F. Weaver
Publikováno v:
Symposium - International Astronomical Union. 20:158-160
In an earlier article* it was pointed out that the galactic radial motions ΔE (R, l) of the very young stars did not show the uniformity of motion to be expected from a smooth regular expansion of the Galaxy. Instead, the very young stars were found
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 161:15P-17P