Results 21 to 30 of about 190,834 (283)
Observational Evidence of the Merging of Filaments and Hub Formation in G083.097+03.270
We uncover a hub–filament system correlated with massive young stellar associations in G083.097+03.270. Diagnosed with simultaneous ^12 CO, ^13 CO, and C ^18 O line observations, the region is found to host two distinct and elongated filaments having ...
Alik Panja +6 more
doaj +1 more source
AbstractOver the past ten years, there has been a revolution in our understanding of massive young stellar clusters in the Galaxy. Initially, there were no known examples having masses >104, yet we now know that there are at least a half dozen such clusters in the Galaxy.
openaire +2 more sources
The Formation and Early Evolution of Young Massive Clusters [PDF]
24 pages, 1 figure. Accepted for publication as a chapter in Protostars and Planets VI, University of Arizona Press (2014), eds. H. Beuther, R. Klessen, C.
S. N. Longmore +9 more
openaire +3 more sources
Infrared photometry of Young Massive Clusters in the starburst galaxy NGC 4214 [PDF]
We present the results of an infrared photometric survey performed with NICS@TNG in the nearby starburst galaxy NGC 4214. We derived accurate integrated JK magnitudes of 10 young massive clusters and compared them with the already available Hubble Space ...
Bragaglia, A. +4 more
core +1 more source
Multiwavelength Observations of Massive Stellar Cluster Candidates in the Galaxy [PDF]
The Galaxy appears to be richer in young, massive stellar clusters than previously known, due to advances in infrared surveys which have uncovered deeply embedded regions of star formation. Young, massive clusters can significantly impact the surrounding
Allen +29 more
core +2 more sources
Structural Properties of Massive Young Clusters [PDF]
We have retrieved multicolor WFPC2/HST data from the STScI archive for 27 nearby Massive (>= 3x10^4 M_Sun) Young (< 20 Myr) star Clusters (MYCs). The data represents the most-complete-to-date sample of clearly resolved MYCs. We have analyzed their structural properties and have found that they can be classified as either Super Star Clusters (SSCs)
Maíz-Apellániz, Jesús +2 more
openaire +2 more sources
To Be or Not to Be: Alicante-8, a Cluster or Not?
Recent surveys have uncovered new young massive clusters that host dozens of red supergiants (RSGs) near the inner Galaxy. However, many of them have still not been fully studied. Using Very Large Telescope/X-shooter near-infrared spectra, we present the
Randa Asa’d +5 more
doaj +1 more source
Formation of Very Young Massive Clusters and Implications for Globular Clusters [PDF]
49 pages, 18 figures, 4 tables. Review chapter to be published in The Origin of Stellar Clusters, ed. S. Stahler (Springer)
Banerjee, Sambaran, Kroupa, Pavel
openaire +2 more sources
In the last decade we have come to realize that the traditional classification of stellar clusters into open and globular clusters cannot be easily extended beyond the realm of the Milky Way, and that even for our Galaxy it is not fully valid. The main failure of the traditional classification is the existence of Massive Young Clusters (MYCs), which ...
openaire +2 more sources
Chemical Abundances of Young Massive Clusters in NGC 1313∗
Abstract We analyze spectroscopic observations of five young massive clusters (YMCs) in the barred spiral galaxy NGC 1313 to obtain detailed abundances from their integrated light. Our sample of YMCs was observed with the X-shooter spectrograph on the Very Large Telescope.
Svea Hernandez +4 more
openaire +4 more sources

