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A dataset of categorized features for the study of transient and seasonal phenomena on the Martian surface. [PDF]
Sci DataNardi A +3 more
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Imbalanced immune cell network and suboptimal cell activation: signatures associated with disease severity in vaccine-naïve COVID-19 patients. [PDF]
Front ImmunolOcaña-Guzman R +9 more
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Adrenal rather than central dysfunction limits hypothalamic-pituitary-adrenal axis recovery after chronic glucocorticoid treatment in male mice. [PDF]
EndocrinologyGaston LS +4 more
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NodoMap: A single-cell and spatial transcriptomic atlas of the mouse nodose ganglion.
Cell Press BlueCheng S +9 more
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Spatial Deconstruction of the Plasma Membrane. [PDF]
J Am Chem SocMandala VS +5 more
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Proceedings of the thirteenth annual symposium on Computational geometry - SCG '97, 1997
We solve two open problems posed by Goodman and Pollack[GP84] about sets of signed circular permutations (clusters of stars) arising from generalized configurations of points: recognition and efficient reconstruction (drawing). As a biproduct we get an O(n2) space data structure constructible in O(n2) time, representing the order type of a (generalized)
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We solve two open problems posed by Goodman and Pollack[GP84] about sets of signed circular permutations (clusters of stars) arising from generalized configurations of points: recognition and efficient reconstruction (drawing). As a biproduct we get an O(n2) space data structure constructible in O(n2) time, representing the order type of a (generalized)
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1982
Astronomy and Astrophysics were first treated in volume III of the 6th edition of Landolt-Bornstein in 1952, then in volumes VI/1 and VI/2 of the New Series, 1965 and 1981/82 respectively. The present volume VI/3 is a further supplementation of volume VI/1.
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Astronomy and Astrophysics were first treated in volume III of the 6th edition of Landolt-Bornstein in 1952, then in volumes VI/1 and VI/2 of the New Series, 1965 and 1981/82 respectively. The present volume VI/3 is a further supplementation of volume VI/1.
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Understanding Stars and Star Clusters
2010Stars are formed from gas and dust compressed together by various forces. Star clusters are formed in several different ways. In what are called open clusters, it is usually the sweeping wave action of the spiral arms of the galaxy thrusting vast stretches of this interstellar material away from the galaxy.
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