Results 61 to 70 of about 399,927 (153)

Immune cells and preterm labour:do invariant NKT cells hold the key? [PDF]

open access: yes, 2015
We have developed our original made-to-measure (M2M) algorithm, PRIMAL, with the aim of modelling the Galactic disc from upcoming Gaia data. From a Milky Way like N-body disc galaxy simulation, we have created mock Gaia data using M0III stars as tracers,
Rinaldi, S F   +3 more
core   +3 more sources

Evidence for fungal proliferation following the Cretaceous/Paleogene mass-extinction event, based on chemostratigraphy in the Raton and Powder River basins, western North America

open access: yesActa Palaeobotanica, 2020
The presence of the amino acid α-aminoisobutyric acid (Aib) within Cretaceous/Paleogene (K/Pg) boundary clay in the Raton and Powder River basins in Colorado and Wyoming, respectively, has been described as compelling evidence that extraterrestrial Aib ...
Keith Berry
doaj   +1 more source

An Integrated Picture of Star Formation, Metallicity Evolution, and Galactic Stellar Mass Assembly

open access: yes, 2008
We present an integrated study of star formation and galactic stellar mass assembly from z=0.05-1.5 and galactic metallicity evolution from z=0.05-0.9 using a very large and highly spectroscopically complete sample selected by rest-frame NIR bolometric ...
A. J. Barger   +4 more
core   +1 more source

Early phase observations of extremely luminous Type Ia Supernova 2009dc [PDF]

open access: yes, 2009
We present early phase observations in optical and near-infrared wavelengths for the extremely luminous Type Ia supernova (SN Ia) 2009dc. The decline rate of the light curve is $\Delta m_{15}(B)=0.65\pm 0.03$, which is one of the slowest among SNe Ia ...
A. Arai   +55 more
core   +2 more sources

Shifts in magnetic mineral assemblages support ocean deoxygenation before the end-Permian mass extinction

open access: yesCommunications Earth & Environment
Expansion of oceanic anoxia is a prevailing hypothesis for driving the marine end-Permian mass extinction and is mainly based on isotopic geochemical proxies.
Min Zhang   +6 more
doaj   +1 more source

The mass function of dense molecular cores and the origin of the IMF [PDF]

open access: yes, 2006
Context: Stars form in the cold dense cores of interstellar molecular clouds and the detailed knowledge of the spectrum of masses of such cores is clearly a key for the understanding of the origin of the IMF. To date, observations have presented somewhat
Alves   +42 more
core   +2 more sources

Stellar populations of galaxies in the ALHAMBRA survey up to $z \sim 1$. II. Stellar content of quiescent galaxies within the dust-corrected stellar mass$-$colour and the $UVJ$ colour$-$colour diagrams

open access: yes, 2019
Our aim is to determine the distribution of stellar population parameters (extinction, age, metallicity, and star formation rate) of quiescent galaxies within the rest-frame stellar mass$-$colour and $UVJ$ colour$-$colour diagrams corrected for ...
A. del Olmo   +30 more
core   +2 more sources

Biogeochemical modeling at mass extinction boundaries [PDF]

open access: yes
The causes of major mass extinctions is a subject of considerable interest to those concerned with the history and evolution of life on earth. The primary objectives of the proposed plan of research are: (1) to develop quantitative time-dependent ...
Caldeira, K. G., Rampino, M. R.
core   +1 more source

Extinctions at 7um and 15um from the ISOGAL survey

open access: yes, 2005
The extinction laws at 7um and 15um are derived for more than 120 sightlines in the inner Galactic plane based on the ISOGAL survey data and the near-infrared data from DENIS and 2MASS. The tracers are the ISOGAL point sources with [7]-[15]
A. Omont   +39 more
core   +2 more sources

Late Frasnian mass extinction: Conodont event stratigraphy, global changes, and possible causes [PDF]

open access: yes
Several abrupt changes in conodont biofacies are documented to occur synchronously at six primary control sections across the Frasnian-Famennian boundary in Euramerica. These changes occurred within a time-span of only about 100,000 years near the end of
Butler, Jamie L.   +3 more
core   +1 more source

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