Results 121 to 130 of about 2,684,722 (398)
How star clusters could survive low star formation efficiencies
, 2004 After the stars of a new, embedded star cluster have formed they blow the remaining gas out of the cluster. Especially winds of high mass stars and definitely the on-set of the first super novae can remove the residual gas from a cluster. This leads to a
Fellhauer, M., Kroupa, P.
core +1 more source
The AIMSS Project I: bridging the star cluster, galaxy divide [PDF]
, 2014 We describe the structural and kinematic properties of the first compact stellar systems discovered by the Archive of Intermediate Mass Stellar Systems project.
M. Norris +17 more
semanticscholar +1 more source
Purification tags markedly affect self‐aggregation of CPEB3
FEBS Letters, EarlyView.Although recombinant proteins are used to study protein aggregation in vitro, uncleaved tags can interfere with accurate interpretation. Our findings demonstrate that His₆‐GFP and His₁₂ tags significantly affect liquid droplet and amyloid fibril formation in the intrinsically disordered region (IDR) of mouse cytoplasmic polyadenylation element‐binding ...
Harunobu Saito +6 more
wiley +1 more source
Chemical evolution of star clusters [PDF]
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2010 I discuss the chemical evolution of star clusters, with emphasis on old Galactic globular clusters (GCs), in relation to their formation histories. GCs are clearly formed in a complex fashion, under markedly different conditions from any younger clusters presently known. Those special conditions must be linked to the early formation epoch of the Galaxy
van Loon, Jacco Th.
openaire +4 more sources
The Transformation of Cluster Galaxies at Intermeidate Redshift
, 2004 We combine imaging data from the Advanced Camera for Surveys (ACS) with VLT/FORS optical spectroscopy to study the properties of star-forming galaxies in the z=0.837 cluster CL0152-1357.
A. R. Martel +46 more
core +1 more source
Circulating histones as clinical biomarkers in critically ill conditions
FEBS Letters, EarlyView.Circulating histones are emerging as promising biomarkers in critical illness due to their diagnostic, prognostic, and therapeutic potential. Detection methods such as ELISA and mass spectrometry provide reliable approaches for quantifying histone levels in plasma samples.
José Luis García‐Gimenez +17 more
wiley +1 more source
Star Cluster Simulations [PDF]
, 2001 The simulation of rich star clusters presents challenging problems of several kinds, including the design of suitable hardware and software, and numerous theoretical problems in stellar dynamics and stellar physics. Great progress has been made possible in recent years through the widespread use of GRAPE hardware.
openaire +3 more sources
Stars, Star Clusters, and Dust in NGC 3077 [PDF]
The Astronomical Journal, 2004 26 pages + 7 postscript figures; to appear in the Astronomical ...
T. J. Davidge +2 more
openaire +5 more sources
Dynamics of Star Cluster Formation: The Effects of Ongoing Star Formation and Stellar Feedback
The Astrophysical JournalWe perform a high-resolution zoomed-in simulation of star cluster assembly including the merger of two subclusters with initial conditions taken from previous large-scale giant molecular cloud (GMC) simulations.
Jeremy Karam +2 more
doaj +1 more source
Do O-stars form in isolation? [PDF]
, 2007 Around 4% of O-stars are observed in apparent isolation, with no associated cluster, and no indication of having been ejected from a nearby cluster. We define an isolated O-star as a star > 17.5 M_\odot in a cluster with total mass 10 M_\odot) stars.
Bastian +25 more
core +3 more sources