M
M. S. N. Kumar
Researcher at University of Porto
Publications - 66
Citations - 2385
M. S. N. Kumar is an academic researcher from University of Porto. The author has contributed to research in topics: Star formation & Stars. The author has an hindex of 26, co-authored 61 publications receiving 2145 citations. Previous affiliations of M. S. N. Kumar include University of Hertfordshire.
Papers
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Journal ArticleDOI
Chemically active outflow L 1157
TL;DR: In this article, the L 1157 bipolar outflow in several molecular emission lines was analyzed and the authors determined the physical characteristics of the CO flow and showed evidence for 3 or 4 independent episodes of mass ejection from the source.
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WFCAM, Spitzer/IRAC and SCUBA observations of the massive star-forming region DR21/W75 - I. The collimated molecular jets
Christopher J. Davis,M. S. N. Kumar,Göran Sandell,Dirk Froebrich,Dirk Froebrich,Michael D. Smith,M. J. Currie +6 more
TL;DR: In this paper, wide-field near-infrared images of the DR21/W75 high-mass star-forming region, obtained with the Wide Field Camera (WFCAM) on the United Kingdom Infrared Telescope, were compared to archival mid-IR images from the Spitzer Space Telescope, and 850-μm dust-continuum maps obtained with SCUBA.
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New Galactic star clusters discovered in the VVV survey
Jura Borissova,Charles Jose Bonatto,R. Kurtev,J. R. A. Clarke,F. Peñaloza,Stuart E. Sale,Stuart E. Sale,Dante Minniti,Dante Minniti,Javier Alonso-García,Étienne Artigau,Rodolfo H. Barbá,Eduardo Luiz Damiani Bica,Gustavo Baume,Márcio Catelan,André-Nicolas Chené,André-Nicolas Chené,Bruno Dias,S. L. Folkes,Dirk Froebrich,Doug Geisler,R. de Grijs,R. de Grijs,Margaret M. Hanson,Maren Hempel,Valentin D. Ivanov,M. S. N. Kumar,P. W. Lucas,Francesco Mauro,C. Moni Bidin,Marina Rejkuba,R. K. Saito,Motohide Tamura,Ignacio Toledo +33 more
TL;DR: In this paper, the authors reported the discovery of 96 new infrared open clusters and stellar groups and derived their fundamental parameters such as reddening, distance, and age by fitting the solar metallicity Padova isochrones to the color-magnitude diagrams.
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A candidate circumbinary Keplerian disk in G35.20-0.74 N: A study with ALMA
Álvaro Sánchez-Monge,R. Cesaroni,Maria T. Beltrán,M. S. N. Kumar,T. Stanke,Hans Zinnecker,Sandra Etoka,D. Galli,Christian A. Hummel,Luca Moscadelli,Thomas Preibisch,Thorsten Ratzka,F. F. S. van der Tak,F. F. S. van der Tak,Sarita Vig,C. M. Walmsley,C. M. Walmsley,K.-S. Wang +17 more
TL;DR: In this paper, two dense cores are detected in typical hot-core tracers (e g, CH3CN) that reveal velocity gradients in one of these cores, the velocity field can be fitted with an almost edge-on Keplerian disk rotating about a central mass of similar to 18 M-circle dot.
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A necklace of dense cores in the high-mass star forming region G35.20−0.74 N: ALMA observations
Álvaro Sánchez-Monge,Álvaro Sánchez-Monge,M. T. Beltrán,Riccardo Cesaroni,Sandra Etoka,Daniele Galli,M. S. N. Kumar,Luca Moscadelli,T. Stanke,F. F. S. van der Tak,Sarita Vig,C. M. Walmsley,C. M. Walmsley,K. S. Wang,Hans Zinnecker,Davide Elia,Sergio Molinari,Eugenio Schisano +17 more
TL;DR: In this paper, the authors used the radio-interferometer ALMA to observe the G35.20−0.74 N region in the submillimeter continuum and line emission at 350 GHz.