1,172 research outputs found
The rationale for attempting to define salt marsh mosquito-breeding areas in Galveston County by remote sensing the associated vegetation
The rationale for attempting to define salt marsh mosquito breeding areas in Galveston County was discussed, including a botanical survey of the marsh plant communities, their relationship to flooding, and their exposure to salt water. Particular emphasis is given to Distichlis spicata, a widespread marsh grass. Evidence suggests that breeding areas of Aedes sollicitans are associated with Distichlis and that both species respond to similar ecological conditions in the salt marsh. Aspects of the remote sensing of the Distichlis are considered
NGC 3628: Ejection Activity Associated with Quasars
NGC3628 is a well-studied starburst/low level AGN galaxy in the Leo Triplet
noted for its extensive outgassed plumes of neutral hydrogen. QSOs are shown to
be concentrated around NGC3628 and aligned with the HI plumes. The closest high
redshift quasar has z=2.15 and is at the tip of an X-ray filament emerging
along the minor axis HI plume. Location at this point has an accidental
probability of ~2x10^-4. In addition a coincident chain of optical objects
coming out along the minor axis ends on this quasar. More recent measures on a
pair of strong X-ray sources situated at 3.2 and 5.4 arcmin on either side of
NGC3628 along its minor axis, reveal that they have nearly identical redshifts
of z=0.995 and 0.981. The closer quasar lies directly in the same X-ray
filament which extends from the nucleus out 4.1 arcmin to end on the quasar of
z=2.15. The chain of objects SW along the minor axis of NGC3628 has been imaged
in four colors with the VLT. Images and spectra of individual objects within
the filament are reported. It is suggested that material in various physical
states and differing intrinsic redshifts is ejected out along the minor axis of
this active, disturbed galaxy.Comment: 8 pages, 5 figures. Accepted for publication in A&A. Postscript file
including full resolution figures at
http://www.eso.org/~fpatat/ngc3628/paper_ngc3628.ps.g
The nature of the ultraluminous X-ray sources inside galaxies and their relation to local QSOs
It is suggested that many of the ultraluminous compact x-ray sources now
being found in the main bodies of galaxies, particularly those that are active,
like M82, NGC 3628 and others, are "local" QSOs, or BL Lac objects, with high
intrinsic redshifts in the process of being ejected from those galaxies.
Evidence in support of this hypothesis is summarized.Comment: submitted to A&A Letter
Meteorological limits on the growth and development of screwworm populations
A program to evaluate the use of remotely sensed data as an additional tool in existing and projected efforts to eradicate the screwworm began in 1973. Estimating weather conditions by use of remotely sensed data was part of the study. Next, the effect of weather on screwworm populations was modeled. A significant portion of the variation in screwworm population growth and development has been traced to weather-related parameters. This report deals with the salient points of the weather and the screwworm population interaction
The ecological variations in thermal infrared emissivity of vegetation
The author has identified the following significant results. Through a series of contrasts, the statistical significance of differences in emissivity was determined for vegegation in dry and humid deserts, montane and deciduous rain forests, and the temperate region. No significant differences were found between the two types of desert vegetation or among the types of nondesert vegetation. However, the rain forest vegetation was significantly different from that of the temperate region. On a community-wide level, there is some physiological adaptation in plants to their radiational environment
System development of the Screwworm Eradication Data System (SEDS) algorithm
The use of remotely sensed data is reported in the eradication of the screwworm and in the study of the role of the weather in the activity and development of the screwworm fly. As a result, the Screwworm Eradication Data System (SEDS) algorithm was developed
The Discovery of a High Redshift X-ray Emitting QSO Very Close to the Nucleus of NGC 7319
A strong X-ray source only 8" from the nucleus of the Sy2 galaxy NGC 7319 in
Stephan's Quintet has been discovered by Chandra. We have identified the
optical counterpart and show it is a QSO with . It is also a ULX
with . From the optical spectra of the QSO
and interstellar gas in the galaxy (z = .022) we show that it is very likely
that the QSO and the gas are interacting.Comment: 8 figures, 5 color, minimized ps siz
The double radio source 3C343.1: A galaxy-QSO pair with very different redshifts
The strong radio source 3C343.1 consists of a galaxy and a QSO separated by
no more than about 0.25 arcsec. The chance of this being an accidental
superposition is conservatively 10^-8. The z=0.344 galaxy is connected to the
z=0.750 QSO by a radio bridge. The numerical relation between the two redshifts
is that predicted from previous associations. This pair is an extreme example
of many similar physical associations of QSOs and galaxies with very different
redshifts.Comment: A&A Letters in pres
Evidence for Intrinsic Redshifts in Normal Spiral Galaxies
The Tully-Fisher Relationship (TFR) is utilized to identify anomalous
redshifts in normal spiral galaxies. Three redshift anomalies are identified in
this analysis: (1) Several clusters of galaxies are examined in which late type
spirals have significant excess redshifts relative to early type spirals in the
same clusters, (2) Galaxies of morphology similar to ScI galaxies are found to
have a systematic excess redshift relative to the redshifts expected if the
Hubble Constant is 72 km s-1 Mpc-1, (3) individual galaxies, pairs, and groups
are identified which strongly deviate from the predictions of a smooth Hubble
flow. These redshift deviations are significantly larger than can be explained
by peculiar motions and TFR errors. It is concluded that the redshift anomalies
identified in this analysis are consistent with previous claims for large
non-cosmological (intrinsic) redshifts.Comment: Accepted for publication at Astrophysics&Space Science. 36 pages
including 8 tables and 7 figure
The Surroundings of Disturbed, Active Galaxies
The brightest apparent magnitude examples of ultra luminous infrared galaxies
(ULIRG's) are studied here in X-ray, optical, infrared and radio wavelengths.
It is is found that they have associated material reaching out to apparent
diameters of the order of a degree on the sky.
Gas, dust, X-ray material and quasars appear to be ejected from the active
nuclei with all objects nearer than their redshift distances.Comment: 14 pages, Figs. 1-28 jpg and gif file
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