A
A. Luna
Researcher at National Institute of Astrophysics, Optics and Electronics
Publications - 45
Citations - 671
A. Luna is an academic researcher from National Institute of Astrophysics, Optics and Electronics. The author has contributed to research in topics: Star formation & Young stellar object. The author has an hindex of 13, co-authored 43 publications receiving 602 citations.
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Journal ArticleDOI
Giant molecular clouds and massive star formation in the southern milky way
Pilar Ortiz García,Pilar Ortiz García,Leonardo Bronfman,Lars-Åke Nyman,Thomas M. Dame,A. Luna +5 more
TL;DR: In this article, the authors used the Columbia University-Universidad de Chile CO Survey of the southern Milky Way to separate the CO(1-0) emission of the fourth Galactic quadrant within the solar circle into its dominant components, giant molecular clouds (GMCs).
Journal ArticleDOI
A Multi-wavelength Study of Star Formation Activity in the S235 Complex
Lokesh K. Dewangan,Lokesh K. Dewangan,Devendra K. Ojha,A. Luna,B. G. Anandarao,Joe P. Ninan,K. K. Mallick,Y. D. Mayya +7 more
TL;DR: In this paper, the authors carried out an extensive multi-wavelength study to investigate the star formation process in the S235 complex, and they found that the Bolocam clump masses increase as we move away from the location of the ionizing star and that the molecular outflows are detected in these three subregions, further confirming the ongoing star formation activity.
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The physical environment of the massive star-forming region w42
TL;DR: In this paper, the authors present an analysis of multi-wavelength observations from various data sets and Galactic plane surveys to study the star-formation process in the W42 complex.
Journal ArticleDOI
Physical environment of massive star-forming region W42
TL;DR: In this paper, the authors present an analysis of multi-wavelength observations from various datasets and Galactic plane surveys to study the star formation process in the W42 complex, showing that a bipolar appearance of W42 is evident due to the ionizing feedback from the O5-O6 type star in a medium that is highly inhomogeneous.
Journal ArticleDOI
Multiwavelength Study of the Star Formation in the S237 H II Region
TL;DR: In this paper, a detailed multi-wavelength study of observations from X-ray, near-infrared, and centimeter wavelengths to probe the star formation processes in the S237 region is presented.