Results 61 to 70 of about 6,328,275 (332)

First evidence of multiple populations along the AGB from Str\"omgren photometry

open access: yes, 2017
Spectroscopic studies have demonstrated that nearly all Galactic globular clusters (GCs) harbour multiple stellar populations with different chemical compositions.
Casagrande, Luca   +5 more
core   +1 more source

Full Three Dimensional Orbits for Multiple Stars on Close Approaches to the Central Supermassive Black Hole [PDF]

open access: yes, 2003
PACS 04A25 With the advent of adaptive optics on the W. M. Keck 10m telescope, two significant steps forward have been taken in building the case for a supermassive black hole at the center of the Milky Way and understanding the black hole’s effect on ...
A. Ghez   +6 more
semanticscholar   +1 more source

Exploring lipid diversity and minimalism to define membrane requirements for synthetic cells

open access: yesFEBS Letters, EarlyView.
Designing the lipid membrane of synthetic cells is a complex task, in which its various roles (among them solute transport, membrane protein support, and self‐replication) should all be integrated. In this review, we report the latest top‐down and bottom‐up advances and discuss compatibility and complexity issues of current engineering approaches ...
Sergiy Gan   +2 more
wiley   +1 more source

Multiple Stellar Populations at Less Evolved Stages. III. A Possible Helium Spread in NGC 2210

open access: yesThe Astrophysical Journal, 2023
Helium variations are common features of globular clusters (GCs) with multiple stellar populations. All the formation scenarios predict that secondary population stars are enhanced in helium, but the exact helium content depends on the polluters ...
Chengyuan Li   +8 more
doaj   +1 more source

General Relativistic Decompression of Binary Neutron Stars During Dynamic Inspiral

open access: yes, 2007
We investigate the dynamic stability of inspiraling neutron stars by performing multiple-orbit numerical relativity simulations of the binary neutron star inspiral process.
Miller, Mark
core   +1 more source

Simulating multiple stars in preparation for Gaia

open access: yesAIP Conference Proceedings, 2011
The scientific preparation of the Gaia mission encompasses both the data reduction algorithms and the generation of simulated data which have to be as realistic as possible.
Frédéric Arenou
semanticscholar   +1 more source

Microbial exopolysaccharide production by polyextremophiles in the adaptation to multiple extremes

open access: yesFEBS Letters, EarlyView.
Polyextremophiles are microorganisms that endure multiple extreme conditions by various adaptation strategies that also include the production of exopolysaccharides (EPSs). This review provides an integrated perspective on EPS biosynthesis, function, and regulation in these organisms, emphasizing their critical role in survival and highlighting their ...
Tracey M Gloster, Ebru Toksoy Öner
wiley   +1 more source

Soft No More: Gas Shielding Protects Soft Binaries from Disruption in Gas-rich Environments

open access: yesThe Astrophysical Journal
Binaries in dense environments are traditionally classified as soft or hard based on their binding energy relative to the kinetic energy of surrounding stars.
Mor Rozner, Hagai B. Perets
doaj   +1 more source

Circumbinary Molecular Rings Around Young Stars in Orion

open access: yes, 2007
We present high angular resolution 1.3 mm continuum, methyl cyanide molecular line, and 7 mm continuum observations made with the Submillimeter Array and the Very Large Array, toward the most highly obscured and southern part of the massive star forming ...
L. A. Zapata   +5 more
core   +1 more source

Massive stars in the giant molecular cloud G23.3−0.3 and W41 [PDF]

open access: yes, 2014
Context. Young massive stars and stellar clusters continuously form in the Galactic disk, generating new Hii regions within their natal giant molecular clouds and subsequently enriching the interstellar medium via their winds and supernovae.Aims. Massive
Aharonian   +121 more
core   +2 more sources

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