ASCA Discovery of an X-ray Pulsar in the Error Box of SGR1900+14

We present a 2 - 10 keV ASCA observation of the field around the soft gamma repeater SGR1900+14. One quiescent X-ray source was detected in this observation, and it was in the SGR error box. In 2 - 10 keV X-rays, its spectrum may be fit by a power law with index -2.2, and its unabsorbed flux is 9.6 x 10^-12 erg cm^-2 s^-1. We also find a clear 5.16 s period. The properties of the three well-studied soft gamma repeaters are remarkably similar to one another, and provide evidence that all of them are associated with young, strongly magnetized neutron stars in supernova remnants.Comment: Accepted for publication in the Astrophysical Journal Letter

Preliminary Parallaxes of 40 L and T Dwarfs from the U.S. Naval Observatory Infrared Astrometry Program

We present preliminary trigonometric parallaxes and proper motions for 22 L dwarfs and 18 T dwarfs measured using the ASTROCAM infrared imager. Relative to absolute parallax corrections are made by employing 2MASS and/or SDSS photometry for reference frame stars. We combine USNO infrared and optical parallaxes with the best available CIT system photometry to determine M_J, M_H, and M_K values for 37 L dwarfs between spectral types L0 to L8 and 19 T dwarfs between spectral types T0.5 and T8 and present selected absolute magnitude versus spectral type and color diagrams, based on these results. Luminosities and temperatures are estimated for these objects. Of special interest are the distances of several objects which are at or near the L-T dwarf boundary so that this important transition can be better understood. The previously reported early-mid T dwarf luminosity excess is clearly confirmed and found to be present at J, H, and K. The large number of objects that populate this luminosity excess region indicates that it cannot be due entirely to selection effects. The T dwarf sequence is extended to M_J~16.9 by 2MASS J041519-0935 which, at d = 5.74 pc, is found to be the least luminous [log(L/L_sun)=-5.58] and coldest (T_eff~760 K) brown dwarf known. Combining results from this paper with earlier USNO CCD results we find that, in contrast to the L dwarfs, there are no examples of low velocity (V_tan < 20 km/s) T dwarfs. We briefly discuss future directions for the USNO infrared astrometry program.Comment: 73 pages, 9 figures, 9 tables, accepted for publication in The Astronomical Journa

Hierarchies and Space Measures for Pointer Machines

Coordinated Science Laboratory was formerly known as Control Systems LaboratoryAir Force Institute of Technology, AFIT/CIR

Efficient On-Line Simulations of Tree Machines and Multidimensional Turing Machines by Random Access Machines

Coordinated Science Laboratory was formerly known as Control Systems LaboratoryOffice of Naval Research / N00014-85-K-0570Air Force Institute of Technolog

Goats to Control the Encroachment of Undesirable Brush and Woody Species in Cattle Pastures

Field studies were initiated in an abandoned, overgrown 8.4 ha orchard left untouched for 15 years to evaluate the effectiveness of using goats (Capra hircus hircus) to manage undesirable vegetation. Goats alone (G: 30 does/ha) or cattle (Bos taurus) with goats (GC:17 does/ha and 3 steers/ha) were mob-grazed twice a year during four grazing seasons. Multiflora rose (Rosa multiflora Thunb.) canopy area decreased from 12 to 2.5 m2 in grazed pastures and multiflora rose live canes were 100% in the control, 0% in G, and only 8% in GC at the completion of the study. Following two years of rest, cattle alone (C: 6 steers) or goats + cattle (GC: 9 goats and 6 steers) were rotationally grazed on the same site. Over four grazing seasons, brambles (Rubus spp.) and honeysuckle (Locifera japonica) vines were practically eliminated from grazed pastures. Multiflora rose bushes grew to a height of 1.8 m in C, but were kept low (avg .6 m) in GC (P \u3c 0.01). Similarly, multiflora rose canopy area was well controlled in GC (avg .5 m2), but increased to 7 m2 in C (P \u3c 0.03). Black locust (Robinia pseudoacacia L.) trees were browsed by goats and cattle and were practically eliminated from grazed pastures. Integrating goats into mountain grazing systems is a useful and environmentally-friendly management tool to keep these pastures in production

The Influence of Growing Degree Days on \u3cem\u3eRobinia Pseudoacacia\u3c/em\u3e Browse Quality and Productivity in the Southeastern USA

The possibility of estimating browse quality and productivity of black locust (BL; Robinia pseudoacacia L.) herbage from accumulated air temperature heat units (growing degree days, GDD) could be a valuable tool for researchers and graziers in efficient allocation of feed resources. Accumulated air temperature heat units (GDD) above a 10° C base have been used to predict several forage quality constituents (Onstad & Fick ,1983)

A ROSAT Deep Survey of Four Small Gamma-Ray Burst Error Boxes

We have used the ROSAT High Resolution Imager to search for quiescent X-ray counterparts to four gamma-ray bursts which were localized to small (< 10 sq. arcmin.) error boxes with the Interplanetary Network. The observations took place years after the bursts, and the effective exposure times for each target varied from ~16 - 23 ks. We have not found any X-ray sources inside any of the error boxes. The 0.1 - 2.4 keV 3 sigma flux upper limits range from around 5 x 10^-14 erg cm^-2 s^-1 to 6 x 10^-13 erg cm^-2 s^-1 depending on the burst and the assumed shape of the quiescent spectrum. We consider four types of X-ray emitting galaxies (normal, AGN, faint, and star-forming) and use the flux upper limits to constrain their redshifts. We then use the GRB fluences to constrain the total energies of the bursts.Comment: 16 pages, 4 figures; submitted to the Astrophysical Journa

A Possible X-Ray Counterpart to SGR 1900+14

The location of the soft gamma repeater SGR 1900ϩ14 was recently reduced to two 15 arcmin2 alternate error boxes by the network synthesis method. We have used the ROSAT High Resolution Imager to observe the error box that is closest to the supernova remnant G42.8ϩ0.6. A quiescent, steady, point X-ray source was found at ␣(2000) ϭ 19h07m14!15, ␦(2000) ϭ 9Њ19Ј19 06, whose unabsorbed flux is 3 ϫ 10Ϫ12 ergs cmϪ2 sϪ1. Its position is also consistent with a peculiar double infrared source described in a companion paper. We have also examined this region using the VLA,1 and have obtained upper limits to the extreme ultraviolet flux of this object using the Extreme-Ultraviolet Explorer