Results 81 to 90 of about 30,812 (255)

Principal sensory experiences of forest visitors in four countries, for evidence‐based nature therapy

People and Nature, Volume 6, Issue 6, Page 2480-2493, December 2024.
Abstract To advance the theoretical and practical underpinnings for nature therapies, i.e. nature exposure as a means to improve mental health, we compared the most memorable sensory experiences reported by forest tourists in Australia, Chile, China and Japan. Sensory experiences are a fundamental driver of the psychological effects of nature exposure.
Ralf C. Buckley, Mary‐Ann Cooper, Linsheng Zhong   +2 more
wiley   +1 more source

Variation in X_CO Factor in N55 Region

Universe
The XCO factor is defined as XCO=N(H2)/W12CO. It is useful for estimating cloud mass. However, there is only limited research on how the XCO factor varies within a single cloud.
Qiang Li, Mingyue Li, Li Zhang, Songpeng Pei   +3 more
doaj   +1 more source

The COS/UVES Absorption Survey of the Magellanic Stream. III: Ionization, Total Mass, and Inflow Rate onto the Milky Way

, 2014
Dynamic interactions between the two Magellanic Clouds have flung large quantities of gas into the halo of the Milky Way, creating the Magellanic Stream, the Magellanic Bridge, and the Leading Arm (collectively referred to as the Magellanic System).
Barger, Kathleen A., Bland-Hawthorn, Joss, Charlton, Jane C., Ely, Justin, Fox, Andrew J., Haffner, L. Matthew, Hernandez, Audra K., Howk, J. Christopher, Kumari, Nimisha, Lehner, Nicolas, Misawa, Toru, Richter, Philipp, Rodriguez-Hidalgo, Paola, Thom, Christopher, Tumlinson, Jason, Wakker, Bart P., Westmeier, Tobias   +16 more
core   +1 more source

Chemical Evolution of the Universe and its Consequences for Gravitational‐Wave Astrophysics

Annalen der Physik, Volume 536, Issue 2, February 2024.
Population properties of double compact object mergers (especially binary black holes) are sensitive to the metallicity dependent cosmic star formation history. The uncertainty of this quantity cannot be ignored and makes the interpretation of current gravitational wave observations difficult.
Martyna Chruślińska
wiley   +1 more source

The 100 Strongest Radio Point Sources in the Field of the Large Magellanic Cloud at 1.4 GHz [PDF]

Serbian Astronomical Journal, 2009
We present the 100 strongest 1.4~GHz point sources from a new mosaicimage in the direction of the Large Magellanic Cloud (LMC). The observationsmaking up the mosaic were made using Australia Telescope Compact Array (ATCA)over a ten year period and were ...
Payne, J. L., Tauber, L. A., Filipović, M. D., Crawford, E. J., De Horta, A. Y.   +4 more
doaj   +3 more sources

The Relevance of Dynamical Friction for the MW/LMC/SMC Triple System

Universe
Simulations of structure formation in the standard cold dark matter cosmological model quantify the dark matter halos of galaxies. Taking into account dynamical friction between dark matter halos, we investigate the past orbital dynamical evolution of ...
Wolfgang Oehm, Pavel Kroupa
doaj   +1 more source

New 6 and 3-cm radio-continuum maps of the Small Magellanic Cloud - part II: Point source catalogue [PDF]

Serbian Astronomical Journal, 2012
We present two new catalogues of radio-continuum sources in the field of the Small Magellanic Cloud (SMC). These catalogues contain sources found at 4800 MHz (λ=6cm) and 8640 MHz (λ=3cm).
Wong G.F., Crawford E.J., Filipović M.D., de Horta A.Y., Tothill N.F.H., Collier J.D., Drašković D., Galvin T.J., Payne J.L.   +8 more
doaj   +1 more source

The WFI Halpha spectroscopic survey of the Magellanic Clouds: Be stars in SMC open clusters [PDF]

, 2008
At low metallicity, B-type stars show lower loss of mass and, therefore, angular momentum so that it is expected that there are more Be stars in the Magellanic Clouds than in the Milky Way.
Baade, Dietrich, Fabregat, Juan, Martayan, Christophe   +2 more
core   +4 more sources

New 20-cm radio-continuum study of the Small Magellanic Cloud, part II: Point sources [PDF]

Serbian Astronomical Journal, 2011
We present a new catalogue of radio-continuum sources in the field of the Small Magellanic Cloud (SMC). This catalogue contains sources previously not found in 2370 MHz (λ=13 cm) with sources found at 1400 MHz (λ=20 cm) and 843 MHz (λ=36 cm). 45
Wong G.F., Filipović M.D., Crawford E.J., Tothill N.F.H., de Horta A.Y., Drašković D., Galvin T.J., Collier J.D., Payne J.L.   +8 more
doaj   +1 more source

Detection of Cold Atomic Clouds in the Magellanic Bridge [PDF]

, 1998
We report a detection of cold atomic hydrogen in the Magellanic Bridge using 21-cm absorption spectroscopy toward the radio source B0312-770. With a column density of N_HI=1.2E20 cm^-2, a maximum absorption optical depth of tau=0.10 and a maximum 21-cm ...
Courtes G., Despois D., Dickey J. M., Henry A. Kobulnicky, Hindman J. V., Israel F. P., John M. Dickey, Johnson P. G., Kalberla P. W. M., Meaburn J., Mebold U., Murai T., Otrupcek R., Pagel B. E. J., Rubio M., Schwering P. B. W., Shapley H.   +16 more
core   +2 more sources