281 research outputs found
Cold as a causal factor in the blood changes due to high altitude
Extracted from The American Journal of the Medical Sciences, August, 1903.https://digitalrepository.unm.edu/unm_bulletin/1012/thumbnail.jp
The effect of altitude upon the blood
https://digitalrepository.unm.edu/unm_bulletin/1036/thumbnail.jp
The potable waters of New Mexico : with special reference to the city water supply
https://digitalrepository.unm.edu/unm_bulletin/1015/thumbnail.jp
The availability of New Mexico\u27s climate for outdoor life
https://digitalrepository.unm.edu/unm_bulletin/1011/thumbnail.jp
Further observations on increased blood counts due to high altitude
https://digitalrepository.unm.edu/unm_bulletin/1013/thumbnail.jp
Some observations on the lung capacity of young people living in New Mexico
https://digitalrepository.unm.edu/unm_bulletin/1035/thumbnail.jp
Pitch Angle Restrictions in Late Type Spiral Galaxies Based on Chaotic and Ordered Orbital Behavior
We built models for low bulge mass spiral galaxies (late type as defined by
the Hubble classification) using a 3-D self-gravitating model for spiral arms,
and analyzed the orbital dynamics as a function of pitch angle, going from
10 to 60. Testing undirectly orbital self-consistency, we search
for the main periodic orbits and studied the density response. For pitch angles
up to approximately , the response supports closely the potential
permitting readily the presence of long lasting spiral structures. The density
response tends to "avoid" larger pitch angles in the potential, by keeping
smaller pitch angles in the corresponding response. Spiral arms with pitch
angles larger than , would not be long-lasting structures but
rather transient. On the other hand, from an extensive orbital study in phase
space, we also find that for late type galaxies with pitch angles larger than
, chaos becomes pervasive destroying the ordered phase space
surrounding the main stable periodic and quasi-periodic orbits and even
destroying them. This result is in good agreement with observations of late
type galaxies, where the maximum observed pitch angle is .Comment: ApJL accepted (12 pages, 3 figures
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