Results 71 to 80 of about 29,943 (214)
An Unbiased CO Survey toward the Northern Region of the Small Magellanic Cloud with the Atacama Compact Array. I. Overview: CO Cloud Distributions [PDF]
, 2021 Kazuki Tokuda +17 more
openalex +1 more source
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 +2 more
wiley +1 more source
Variation in XCO Factor in N55 Region
UniverseThe 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 +3 more
doaj +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 Relevance of Dynamical Friction for the MW/LMC/SMC Triple System
UniverseSimulations 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
The sub-solar Initial Mass Function in the Large Magellanic Cloud
, 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
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 +2 more
core +4 more sources
New 20-cm radio-continuum study of the small Magellanic cloud - part III: Compact Hii regions [PDF]
Serbian Astronomical Journal, 2012 We present and discuss a new catalogue of 48 compact Hii regions in the Small Magellanic Cloud (SMC) and a newly created deep 1420 MHz (λ=20 cm) radio-continuum image of the N19 region located in the southwestern part of the SMC.
Wong G.F. +5 more
doaj +1 more source
The Astrophysical JournalThe 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
, 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