552 research outputs found
Alien Registration- West, Frederick (Limestone, Aroostook County)
https://digitalmaine.com/alien_docs/35218/thumbnail.jp
Who Are The Christian Churches And What Do We Believe?
https://digitalcommons.acu.edu/crs_books/1488/thumbnail.jp
A method of evaluating efficiency during space-suited work in a neutral buoyancy environment
The purpose was to investigate efficiency as related to the work transmission and the metabolic cost of various extravehicular activity (EVA) tasks during simulated microgravity (whole body water immersion) using three space suits. Two new prototype space station suits, AX-5 and MKIII, are pressurized at 57.2 kPa and were tested concurrently with the operationally used 29.6 kPa shuttle suit. Four male astronauts were asked to perform a fatigue trial on four upper extremity exercises during which metabolic rate and work output were measured and efficiency was calculated in each suit. The activities were selected to simulate actual EVA tasks. The test article was an underwater dynamometry system to which the astronauts were secured by foot restraints. All metabolic data was acquired, calculated, and stored using a computerized indirect calorimetry system connected to the suit ventilation/gas supply control console. During the efficiency testing, steady state metabolic rate could be evaluated as well as work transmitted to the dynamometer. Mechanical efficiency could then be calculated for each astronaut in each suit performing each movement
The Brown Dwarf Kinematics Project (BDKP). III. Parallaxes for 70 Ultracool Dwarfs
We report parallax measurements for 70 ultracool dwarfs (UCDs). Using both
literature values and our sample, we report new polynomial relations between
spectral type and M. Including resolved L/T transition binaries in the
relations, we find no reason to differentiate between a "bright" (unresolved
binary) and "faint" (single source) sample across the L/T boundary. Isolating
early T dwarfs, we find that the brightening of T0-T4 sources is prominent in
M where there is a [1.2 - 1.4] magnitude difference. A similar yet
dampened brightening of [0.3 - 0.5] magnitude happens at M and a plateau
or dimming of [-0.2 - -0.3] magnitude is seen in M. Comparing with
evolutionary models that vary gravity, metallicity, and cloud thickness we find
that a near constant temperature of 1200 100 K along a narrow spectral
subtype of T0-T4 is required to account for the brightening and color magnitude
diagram of the L-dwarf/T-dwarf transition. Furthermore, there is a significant
population of both L and T dwarfs which are red or potentially "ultra-cloudy"
compared to the models, many of which are known to be young indicating a
correlation between enhanced photospheric dust and youth. For the low
surface-gravity or young companion L dwarfs we find that 8 out of 10 are at
least [0.2-1.0] magnitude underluminous in M and/or M compared to
equivalent spectral type objects. We speculate that this is a consequence of
increased dust opacity and conclude that low-surface gravity L dwarfs require a
completely new spectral-type/absolute magnitude polynomial for analysis.Comment: 65 pages, Accepted for publication to Ap
Prediction of optimal flight profiles for jet aircraft under short range and low fuel conditions.
http://www.archive.org/details/predictionofopti00wes
The Brown Dwarf Kinematics Project (BDKP). II. Details on Nine Wide Common Proper Motion Very Low-Mass Companions to Nearby Stars
We report on nine wide common proper motion systems containing late-type M,
L, or T companions. We confirm six previously reported companions, and identify
three new systems. The ages of these systems are determined using diagnostics
for both stellar primaries and low--mass secondaries and masses for the
secondaries are inferred using evolutionary models. Of our three new
discoveries, the M3+T6.5 pair G 204-39 and SDSS J1758+4633 has an age
constrained to 0.5-1.5 Gyr making the secondary a potentially useful brown
dwarf benchmark. The G5+L4 pair G 200-28 and SDSS J1416+5006 has a projected
separation of ~25,000 AU making it one of the widest and lowest binding energy
systems known to date. The system containing NLTT 2274 and SDSS J0041+1341 is
an older M4+L0 (>4.5 Gyr) pair which shows Halpha activity in the secondary but
not the primary making it a useful tracer of age/mass/activity trends. We find
a resolved binary frequency for widely-separated (> 100 AU) low--mass
companions (i.e. at least a triple system) which is at least twice the
frequency found for the field ultracool dwarf population. The ratio of triples
to binaries and quadruples to binaries is also high for this sample: 3:5 and
1:4, respectively, compared to 8-parsec sample values of 1:4 and 1:26. The
additional components in these wide companion systems indicates a formation
mechanism that requires a third or fourth component to maintain gravitational
stability or facilitate the exchange of angular momentum. The binding energies
for the nine multiples discussed in this text are among the lowest known for
wide low-mass systems, suggesting that weakly bound, low--to--intermediate mass
(0.2M_sun < M_tot <1.0M_sun) multiples can form and survive to exist in the
field (1-8 Gyr).Comment: 62 pages, 12 figures, 11 Tables, AJ accepted for publicatio
Can conversational interviewing improve survey response quality without increasing interviewer effects?
Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/141370/1/rssa12255_am.pdfhttps://deepblue.lib.umich.edu/bitstream/2027.42/141370/2/rssa12255.pd
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