95 research outputs found
UV sky surveys
I review the development of UV and EUV astronomy, covering the spectral range
from 5 to 300 nm, with emphasis on sky surveys for discrete sources. I discuss
studies which resulted in lists of sources observed by imaging and deliberately
omit most spectroscopic studies. Technical issues, such as detector and
telescope developments, are treated separately from descriptions of specific
missions and their results, which contributed to the understanding of the UV
sky. The missions are compared in terms of their ``survey power'', a variable
which combines sky coverage and survey depth. I use the existing knowledge of
UV sources to predict views of the UV sky, which I then compare with those
actually detected. Finally, UV missions which will detect fainter sources and
will fly in the near future are described, and a wish list for low-cost
ventures, which could advance considerably our knowledge of the UV sky is
presented.Comment: 53 pages, 11 figures, accepted by Experimental Astronomy, uses
crckapb.sty (style file from Kluwer
Galaxy interactions in the Hickson Compact Group 88
I present observations of the Hickson Compact Group 88 (HCG88) obtained
during the commissioning of a new 28-inch telescope at the Wise Observatory.
This galaxy group was advertised to be non-interacting, or to be in a very
early interaction stage, but this is not the case. The observations reported
here were done using a "luminance" filter, essentially a very broad R filter,
reaching a low surface brightness level of about 26 mag per square arcsec.
Additional observations were obtained in a narrow spectral band approximately
centered on the rest-frame H-alpha line from the group. Contrary to previous
studies, my observations show that at least two of the major galaxies have had
significant interactions in the past, although probably not between themselves.
I report the discovery of a faint extended tail emerging from the brightest of
the group galaxies, severe isophote twisting and possible outer shells around
another galaxy, and map the HII regions in all the galaxies.Comment: 17 pages, 3 figures. MNRAS, in pres
Thinking about Archeoastronomy
I discuss various aspects of archeoastronomy concentrating on physical
artifacts (i.e., not including ethno-archeoastronomy) focusing on the period
that ended about 2000 years ago. I present examples of artifacts interpreted as
showing the interest of humankind in understanding celestial phenomena and
using these to synchronize calendars and predict future celestial and
terrestrial events. I stress the difficulty of identifying with a high degree
of confidence that these artifacts do indeed pertain to astronomy and caution
against the over-interpretation of the finds as definite evidence.
With these in mind, I point to artifacts that seem to indicate a human
fascination with megalithic stone circles and megalithic alignments starting
from at least 11000 BCE, and to other items presented as evidence for Neolithic
astronomical interests dating to even 20000 BCE or even before. I discuss the
geographical and temporal spread of megalithic sites associated with
astronomical interpretations searching for synchronicity or for a possible
single point of origin.
A survey of a variety of artifacts indicates that the astronomical
development in antiquity did not happen simultaneously at different locations,
but may be traced to megalithic stone circles and other megalithic structures
with possible astronomical connections originating in the Middle East,
specifically in the Fertile Crescent area. The effort of ancient societies to
erect these astronomical megalithic sites and to maintain a corpus of astronomy
experts does not appear excessive.Comment: 28 pages, three figures, extended contribution to the archeoastronomy
workshop held at IMeRA, Marseille on November 30, 201
Grey Milky Way Extinction from SDSS Stellar Photometry
We report results concerning the distribution and properties of galactic
extinction at high galactic latitudes derived from stellar statistics using the
Sloan Digital Sky Survey (SDSS). We use the classical Wolf diagram method to
identify regions with extinction, and derive the extinction and the extinction
law of the dust using all five SDSS spectral bands. We estimate the distance to
the extinguishing medium using simple assumptions about the stellar populations
in the line of sight.
We report the identification of three extinguishing clouds, each a few tens
of pc wide, producing 0.2-0.4 mag of g'-band extinction, located 1-2 kpc away
or 0.5-1 kpc above the galactic plane. All clouds exhibit grey extinction,
i.e., almost wavelength-independent in the limited spectral range of the SDSS.
We discuss the implication of this finding on general astrophysical questions.Comment: 30 pages, 13 figures. Accepted for publication in MNRA
Normal Galaxies - INES Guide No. 2
This guide presents, in a uniform manner, all the information collected by
the IUE satellite on normal galaxies. It contains information on 274 galaxies
and it supersedes the previous IUE guide to normal galaxies (Longo & Capaccioli
1992). The data shown here are restricted to galaxies defined as ``normal'' by
the observer, and entered as such in the IUE data file header. The information
is also restricted to low-dispersion spectra obtained through the large
apertures of IUE. For the first time, we provide spectral information from
well-defined and identifiable locations in the target galaxies. These are
mostly located close to the photocenter of each object, although there are few
exceptions. Each representative spectrum of a galaxy consists of a short-wave
(SW) and a long-wave (LW) IUE low-dispersion spectrum (where available)
combined into a single spectrum covering the wavelength range 1150 A to 3350 A.
We selected the two spectra to be combined so as to be, preferably, the deepest
exposures available in the INES archive. Each representative spectrum is
accompanied by two images of the galaxy, on which the locations of the SW
entrance aperture and the LW entrance aperture are marked. The guide is
available at (http://wise-iue.tau.ac.il/~lili/Fnet/Fnet.html)Comment: 36 pages, 7 figures. INES Access Guide N.2-ESA SP-1239 2000.
Noordwijk:ESA Publ. Dep. The full atlas is available on line at
http://wise-iue.tau.ac.il/~lili/Fnet/Fnet.htm
A Simple Isolation Criterion based on 3D Redshift Space Mapping
We selected a sample of galaxies, extremely isolated in 3D redshift space,
based on data from NED and the ongoing ALFALFA HI (21cm) survey. A simple
selection criterion was employed: having no neighbors closer than 300 km/s in
3D redshift space. The environments of galaxies, selected using this criterion
and NED data alone, were analyzed theoretically using a constrained simulation
of the local Universe, and were found to be an order of magnitude less dense
than environments around randomly selected galaxies. One third of the galaxies
selected using NED data alone did not pass the criterion when tested with
ALFALFA data, implying that the use of unbiased HI data significantly improves
the quality of the sample.Comment: 4 pages, 2 figures. To be published in the proceedings of the
conference "Galaxies in Isolation: Exploring Nature vs. Nurture", Granada,
12-15 May 200
Many binaries among NEAs
The number of binary asteroids in the near-Earth region might be
significantly higher than expected. While Bottke and Melosh (1996) suggested
that about 15% of the NEAs are binaries, as indicated from the frequency of
double craters, and Pravec and Harris (2000) suggested that half of the
fast-rotating NEAs are binaries, our recent study of Aten NEA lightcurves shows
that the fraction of binary NEAs might be even higher than 50%. We found two
asteroids with asynchronous binary characteristics such as two additive periods
and fast rotation of the primary fragment. We also identified three asteroids
with synchronous binary characteristics such as amplitude higher than one
magnitude, U-shaped lightcurve maxima and V-shaped lightcurve minima. These
five binaries were detected out of a sample of eight asteroids observed,
implying a 63% binarity frequency. Confirmation of this high binary population
requires the study of a larger representative sample. However, any mitigation
program that requires the deflection or demise of a potential impactor will
have to factor in the possibility that the target is a binary or multiple
asteroid system.Comment: 5 pages, 2 figures, invited paper for NASA's "Near-Earth Object
Detection, Characterization, and Threat Mitigation" workhop, Colorado, June
200
Quest for truly isolated galaxies
I describe attempts to identify and understand the most isolated galaxies
starting from my 1983 Leiden PhD thesis, continuing through a string of
graduate theses on various aspects of this topic, and concluding with an
up-to-date account of the difficulty to find really isolated objects. The
implication of some of the findings revealed on the way and presented here is
that the nearby Universe may contain many small dark-matter haloes, and that
some such haloes may possibly be accreting intergalactic gas to form dwarf
galaxies.Comment: Contribution for the "Galaxies in Isolation" conferenc
Star Formation in Dwarf Galaxies
We explore mechanisms for the regulation of star formation in dwarf galaxies.
We concentrate primarily on a sample in the Virgo cluster, which has HI and
blue total photometry, for which we collected H data at the Wise
Observatory. We find that dwarf galaxies do not show the tight correlation of
the surface brightness of H (a star formation indicator) with the HI
surface density, or with the ratio of this density to a dynamical timescale, as
found for large disk or starburst galaxies. On the other hand, we find the
strongest correlation to be with the average blue surface brightness,
indicating the presence of a mechanism regulating the star formation by the
older (up to 1 Gyr) stellar population if present, or by the stellar population
already formed in the present burst.Comment: 15 pages (LATEX aasms4 style) and three postscript figures, accepted
for publication in the Astrophysical Journa
Late-Type Dwarf Galaxies in the Virgo Cluster: I. The Samples
We selected samples of late-type dwarf galaxies in the Virgo cluster with HI
information. The galaxies were observed at the Wise-Observatory using several
broad-band and H bandpasses. UV measurements were carried out with the
IUE Observatory from VILSPA, and with the FAUST shuttle-borne UV telescope.
We describe our observations in detail, paying particular attention to the
determination of measurement errors, and present the observational results
together with published data and far-infrared information from IRAS. The sample
will be analyzed in subsequent papers, in order to study star formation
mechanisms.Comment: Modified version, accepted for publication in MNRAS, 26 page
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