Results 271 to 280 of about 17,995 (289)

Proteome-Wide Analysis and Surface Protein Isolation for Secretome Characterization Reveal Insights into the Biology of the Leaf-Cutter Ant <i>Acromyrmex echinatior</i>. [PDF]

Anal Chem
Huang P, Sardina J, Lu H, Bruner-Montero G, Currie CR, Li L.   +5 more
europepmc   +1 more source

Formation of a low-mass galaxy from star clusters in a 600-million-year-old Universe. [PDF]

Nature
Mowla L, Iyer K, Asada Y, Desprez G, Tan VYY, Martis N, Sarrouh G, Strait V, Abraham R, Bradač M, Brammer G, Muzzin A, Pacifici C, Ravindranath S, Sawicki M, Willott C, Estrada-Carpenter V, Jahan N, Noirot G, Matharu J, Rihtaršič G, Zabl J.   +21 more
europepmc   +1 more source

Formation of free-floating planetary mass objects via circumstellar disk encounters. [PDF]

Sci Adv
Fu Z, Deng H, Lin DNC, Mayer L.
europepmc   +1 more source

Comparative genomic analysis of the MAPKKK gene family reveals WGD-driven expansion and strong evolutionary constraints in Asteraceae. [PDF]

Front Plant Sci
Chen Y, Han Z, Peng R, Zhang C.
europepmc   +1 more source

Midbrain extracellular matrix and microglia are associated with cognition in aging mice. [PDF]

Nat Commun
Gray DT, Gutierrez A, Jami-Alahmadi Y, Pandey V, Pan L, Zhang Y, Wohlschlegel JA, McDevitt RA, De Biase LM.   +8 more
europepmc   +1 more source

Young, Massive Star Clusters in the Antennae [PDF]

, 2008
While massive star clusters have been detected in almost every galaxy with appreciable star formation, they are most prevalent in interacting and merging galaxies. As many as 95% of these clusters will ultimately be disrupted, often in the first 10 Myr, but those clusters that do survive may be the progenitors of globular clusters.
Christopher, Micol Huw
openaire   +3 more sources

Massive binary stars and the kinematics of Young Massive Clusters [PDF]

, 2013
Located in the Large Magellanic Cloud, R136 is a rare example of a nearby young and dense massive star cluster in which individual stars can be resolved. Often suggested as a globular cluster in formation, its study is of great interest and promises to provide insights into the early dynamical evolution of massive star clusters.
Henault-Brunet, Vincent, Brunet, Vincent
openaire   +3 more sources

Gas expulsion and the destruction of massive young clusters [PDF]

Monthly Notices of the Royal Astronomical Society, 2006
We examine the luminosity and dynamical mass estimates for young massive stellar clusters. For many young (
Simon P Goodwin, N Bastian, Goodwin Simon P   +2 more
exaly   +3 more sources

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Young massive clusters in Arp 299

Proceedings of the International Astronomical Union, 2019
AbstractBecause of their young ages and compact densities, young massive star clusters (YMCs) are widely considered as potential proto-globular clusters. They are ubiquitous in environments with ongoing star formation activity such as interacting luminous infrared galaxies.
Zara Randriamanakoto, Petri Väisänen
openaire   +1 more source