Results 71 to 80 of about 30,329 (257)

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

open access: yesPeople 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   +2 more
wiley   +1 more source

Spatial motion of the Magellanic Clouds. Tidal models ruled out?

open access: yes, 2008
Recently, Kallivayalil et al. derived new values of the proper motion for the Large and Small Magellanic Clouds (LMC and SMC, respectively). The spatial velocities of both Clouds are unexpectedly higher than their previous values resulting from agreement
Palous, Jan   +2 more
core   +1 more source

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

open access: yes, 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.   +16 more
core   +2 more sources

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

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

open access: yesSerbian 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.   +8 more
doaj   +1 more source

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

open access: yesAnnalen 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 sub-solar Initial Mass Function in the Large Magellanic Cloud

open access: yes, 2008
The Magellanic Clouds offer a unique variety of star forming regions seen as bright nebulae of ionized gas, related to bright young stellar associations.
Gouliermis, Dimitrios A.
core   +1 more source

Mapping atomic and diffuse interstellar band absorption across the Magellanic Clouds and the Milky Way [PDF]

open access: yes, 2015
Diffuse interstellar bands (DIBs) trace warm neutral and weakly-ionized diffuse interstellar medium (ISM). Here we present a dedicated, high signal-to-noise spectroscopic study of two of the strongest DIBs, at 5780 and 5797 \AA, in optical spectra of 666
Bailey, Mandy   +3 more
core   +2 more sources

UVIT Study of the Magellanic Clouds (U-SMAC). III. Hierarchical Star Formation in the Small Magellanic Cloud Regulated by Turbulence

open access: yesThe Astrophysical Journal
The Small Magellanic Cloud (SMC), a satellite galaxy of the Milky Way, is an irregular dwarf galaxy exhibiting evidence of recent and ongoing star formation.
Sipra Hota   +2 more
doaj   +1 more source

High Excitation Molecular Gas in the Magellanic Clouds

open access: yes, 2005
We present the first survey of submillimeter CO 4-3 emission in the Magellanic Clouds. The survey is comprised of 15 6'x6' maps obtained using the AST/RO telescope toward the molecular peaks of the Large and Small Magellanic Clouds.
Alberto D. Bolatto   +15 more
core   +1 more source

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