122 research outputs found

    Review Essay

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    The Princeton Project on National Security describes itself as a “three-year, bi- partisan initiative to develop a sustainable and effective national security strat- egy for the United States of America.” Consisting of the final report and seven working group reports (on Grand Strategic Choices, State Security and Trans- national Threats, Economics and National Security, Reconstruction and Development, Anti-Americanism, Relative Threat Assessment, and Foreign Infrastruc- ture and Global Institutions), this study, like so many others, wrestles with the great unresolved problem that plagues contemporary policy makers and schol- ars: What is the central organizing principle behind American national security policy

    Seapower and Space: From the Dawn of the Missile Age toNet-centric Warfare,

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    This work examines the development of space systems and its implications for naval warfare in the twenty-first century by focusing on the argument that “access to space systems makes possible a new style of warfare.” It addresses the “linked revolution of long-range missiles and their space-based supporting systems.” Furthermore, Friedman seeks to under- stand how the development of space- based systems (notably rockets and satellites) has radically influenced how naval forces conduct navigation, communication, reconnaissance, and targeting. The reality is that modern military forces depend almost entirely on platforms in space to know where they are and to communicate with friendly forces, as well as to know the location of enemy forces and use that information to destroy them. This “rev- olution in military affairs” is now hav- ing an effect on a global scale

    Review Essay—Technologies That May Yet Revolutionize WarfareFuture Wars Will Be Fought

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    The E-Bomb: How America’s New Directed Energy Weapons Will Change the Way Future Wars Will Be Fough

    Grand Strategy in Theory and Practice

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    Victory in War: Foundations of Modern Military Policy

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    The Extended Line Region of 3C 299

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    We present results of HST observations of the radio galaxy 3C 299. The broad-band F702W (R) and F555W (V) images (WFPC2/PC) show an elliptical galaxy, with a comet-like structure extending to the NE in the radio jet direction. The [OIII]λ\lambda5007 emission line map, shows a bi-conical structure centered on the nucleus, that overlaps the structure found in the broad-band filters. The radio core coincides with the center of the bi-conical structure and the radio axes are aligned with the direction of the cones. These data show clear evidence of a strong interaction between the radio jet and the NE morphology of the galaxy. We show evidence that this NE region is an ENLR; the line-ratio diagnostics show that models involving gas shocked by the radio-jet plus ionization from a precursor HII region, produced itself by the ionizing photons of the postshocked gas on the preshocked gas provide a good match to the observations. We investigate the spatial behavior of the ionizing parameter UU, by determining the [OIII]/[OII] line ratio which is sensitive to the change of the ionization parameter, and trace its behavior over the ENLR along the radio jet direction. We find that [OIII]/[OII] does not follow a simple dilution model, but rather that it is approximately constant over a large range of distance from the nucleus thus requiring a local source of ionization which seems to be compatible with the shock models driven by the radio jet.Comment: 17 pages, 9 Postscript figures, ApJ accepted, uses aaspp.st

    3C236: Radio Source, Interrupted?

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    We present new HST STIS/MAMA near-UV images and archival WFPC2 V and R band images which reveal the presence of four star forming regions in an arc along the edge of the dust lane in the giant (4 Mpc) radio galaxy 3C236. Two of the star forming regions are relatively young with ages of order 1E7 yr, while the other two are older with ages of order 1E8 - 1E9 yr which is comparable to the estimated age of the giant radio source. Based on dynamical and spectral aging arguments, we suggest that the fuel supply to the AGN was interrupted for 1E7 yr and has now been restored, resulting in the formation of the inner 2 kpc scale radio source. This time scale is similar to that of the age of the youngest of the star forming regions. We suggest that the transport of gas in the disk is non-steady and that this produces both the multiple episodes of star formation in the disk as well as the multiple epochs of radio source activity. If the inner radio source and the youngest star forming region are related by the same event of gas transport, the gas must be transported from the hundreds of pc scale to the sub-parsec scale on a time scale of 1E7 yr, which is similar to the dynamical time scale of the gas on the hundreds of pc scales

    Discovery of Two Distant Type Ia Supernovae in the Hubble Deep Field North with the Advanced Camera for Surveys

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    We present observations of the first two supernovae discovered with the recently installed Advanced Camera for Surveys (ACS) on the Hubble Space Telescope. The supernovae were found in Wide Field Camera images of the Hubble Deep Field North taken with the F775W, F850LP, and G800L optical elements as part of the ACS guaranteed time observation program. Spectra extracted from the ACS G800L grism exposures confirm that the objects are Type Ia supernovae (SNe Ia) at redshifts z=0.47 and z=0.95. Follow-up HST observations have been conducted with ACS in F775W and F850LP and with NICMOS in the near-infrared F110W bandpass, yielding a total of 9 flux measurements in the 3 bandpasses over a period of 50 days in the observed frame. We discuss many of the important issues in doing accurate photometry with the ACS. We analyze the multi-band light curves using two different fitting methods to calibrate the supernovae luminosities and place them on the SNe Ia Hubble diagram. The resulting distances are consistent with the redshift-distance relation of the accelerating universe model, although evolving intergalactic grey dust remains as a less likely possibility. The relative ease with which these SNe Ia were found, confirmed, and monitored demonstrates the potential ACS holds for revolutionizing the field of high-redshift SNe Ia, and therefore of testing the accelerating universe cosmology and constraining the "epoch of deceleration".Comment: 11 pages, 8 embedded figures. Accepted for publication in Ap
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