Feedback from massive stars and gas expulsion from proto-globular clusters [PDF]
© 2015. The American Astronomical Society. All rights reserved. Globular clusters (GCs) are considerably more complex structures than previously thought, harboring at least two stellar generations that present clearly distinct chemical abundances ...
Calura, F. +3 more
core +3 more sources
A Census of the Circumstellar Disk Populations in the Sco-Cen Complex
I have used mid-infrared (IR) photometry from the Wide-field Infrared Survey Explorer (WISE) to perform a census of circumstellar disks among ∼10,000 candidate members of the Sco-Cen complex that were recently identified with data from the Gaia mission ...
K. L. Luhman
doaj +1 more source
Isolated OB Associations in Stripped HI Gas Clouds
HST ACS/HRC images in UV (F250W), V (F555W), and I (F814W) resolve three isolated OB associations that lie up to 30 kpc from the stellar disk of the S0 galaxy NGC 1533.
Chiosi C. +12 more
core +1 more source
A multiphysics and multiscale software environment for modeling astrophysical systems [PDF]
We present MUSE, a software framework for combining existing computational tools for different astrophysical domains into a single multiphysics, multiscale application.
Andrea Sottoriva +66 more
core +2 more sources
Massive runaway stars in the Small Magellanic Cloud [PDF]
Using archival Spitzer Space Telescope data, we identified for the first time a dozen runaway OB stars in the Small Magellanic Cloud (SMC) through the detection of their bow shocks.
Bica +63 more
core +2 more sources
The distinction between star clusters and associations
In Galactic studies a distinction is made between (open) star clusters and associations. For barely resolved objects at a distance of several Mpc this distinction is not trivial to make. Here we provide an objective definition by comparing the age of the
Ambartsumian +10 more
core +1 more source
Lower limit for differential rotation in members of young loose stellar associations [PDF]
Surface differential rotation (SDR) plays a key role in dynamo models. SDR estimates are therefore essential for constraining theoretical models. We measure a lower limit to SDR in a sample of solar-like stars belonging to young associations with the aim
Distefano, E. +4 more
core +2 more sources
Six More Ultra-faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey
We report the discovery of six ultra-faint Milky Way satellites identified through matched-filter searches conducted using Dark Energy Camera (DECam) data processed as part of the second data release of the DECam Local Volume Exploration (DELVE) survey ...
W. Cerny +33 more
doaj +1 more source
Mapping the Recent Star Formation History of the Disk of M51
Using data acquired as part of a unique Hubble Heritage imaging program of broadband colors of the interacting spiral system M51/NGC 5195, we have conducted a photometric study of the stellar associations across the entire disk of the galaxy in order to ...
Brown +19 more
core +1 more source
The embedded cluster or association Trumpler 37 in IC1396: a search for evolutionary constraints [PDF]
It is currently widely accepted that open star clusters and stellar associations result from the evolution of embedded star clusters. Parameters such star formation efficiency, time-scale of gas removal and velocity dispersion can be determinants of ...
Bica, E., Bonatto, C., Saurin, T. A.
core +2 more sources

