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The VMC Survey. XXVII. Young Stellar Structures in the LMC's Bar Star-forming Complex
(IOP Publishing, 2017-11)
Star formation is a hierarchical process, forming young stellar structures of star clusters, associations, and complexes over a wide range of scales. The star-forming complex in the bar region of the Large Magellanic Cloud ...
Spectro-interferometric observations of a sample of Be stars: Setting limits to the geometry and kinematics of stable Be disks
(EDP Sciences, 2019-01)
Context. Be stars are rapid rotators surrounded by a gaseous disk envelope whose origin is still under debate. This envelope is responsible for observed emission lines and large infrared excess. Aims. To progress in the ...
Molecular gas, kinematics, and OB star formation in the spiral arms of the southern Milky Way
(UNIV CHICAGO PRESS, 2006-04-20)
The rotation curve for the fourth Galactic quadrant within the solar circle is derived from the Columbia University - Universidad de Chile CO (J = 1 -> 0) survey of molecular gas. A new sampling, 4 times denser in longitude ...
The Taurus Boundary of stellar/substellar (TBOSS) survey. II. Disk masses from ALMA continuum observations
(IOP Publishing Ltd, 2018)
We report 885 mu m ALMA continuum flux densities for 24 Taurus members spanning the stellar/substellar boundary with spectral types from M4 to M7.75. Of the 24 systems, 22 are detected at levels ranging from 1.0 to 55.7 ...
ALMA [N II] 205 mu m Imaging Spectroscopy of the Interacting Galaxy System BRI 1202-0725 at Redshift 4.7
(IOP PUBLISHING LTD, 2017)
We present the results from Atacama Large Millimeter/submillimeter Array imaging in the [N II] 205 mu m fine-structure line (hereafter [N II]) and the underlying continuum of BRI 1202-0725, an interacting galaxy system at ...
Eeffect of feedback of massive stars in the fragmentation, distribution, and kinematics of the gas in two star forming regions in theCarina nebula
(IOP, 2020)
We present ALMA high spatial resolution observations toward two star-forming regions located in one of the most extreme zones of star formation in the Galaxy, the Carina Nebula. One region is located at the center of the ...
ALMA Reveals Sequential High-mass Star Formation in the G9.62+0.19 Complex
(IOP Publishing Ltd, 2017)
Stellar feedback from high-mass stars (e.g., H II regions) can strongly influence the surrounding interstellar medium and regulate star formation. Our new ALMA observations reveal sequential high-mass star formation taking ...
Star formation along the Hubble sequence Radial structure of the star formation of CALIFA galaxies
(EDP Sciences, 2016)
The spatially resolved stellar population content of today's galaxies holds important information for understanding the different processes that contribute to the star formation and mass assembly histories of galaxies. The ...