Vineet Rawat
5 Papers
Vineet Rawat is an academic researcher. The author has contributed to research in topics: Star formation & Paleontology. The author has co-authored 2 publications.
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Papers
The Giant Molecular Cloud G148.24+00.41: Gas Properties, Kinematics, and Cluster Formation at the Nexus of Filamentary Flows
Vineet Rawat,Manash R. Samal,D. L. Walker,D. K. Ojha,Anandmayee Tej,Annie Zavagno,C. P. Zhang,D. Elia,S. Dutta,J. Jose,Chakali Eswaraiah,E. S. P. R. Laboratory,Indian Institute of Technology Gandhinagar,J. B. C. F. Astrophysics,T. I. O. F. Research,Indian Institute of Space Science,Technology,Aix-Marseille Universite,I. France,National Astronomical Observatories,Chinese Academy of Sciences,Guizhou Radio Astronomical Observatory,Guizhou University,Istituto di Astrofisica e Planetologia Spaziali,I. O. Astronomy,Astrophysics,A. Sinica,Indian Institute of Science Education,Research Tirupati +28 more
TL;DR: G148.24+00.41 is a massive molecular cloud with filamentary flows and cluster formation. The cloud is massive and has fragmented into clumps. Filamentary flows are converging towards the central area of the cloud and transferring mass to the clumps.
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Probing the Global Dust Properties and Cluster Formation Potential of the Giant Molecular Cloud G148.24+00.41
Vineet Rawat,Manash R. Samal,Daniel Walker,Annie Zavagno,Anandmayee Tej,Gábor Marton,D. K. Ojha,D. Elia,W. P. Chen,Jessy Jose,Chakali Eswaraiah +10 more
TL;DR: In this paper , the authors make use of CO, Herschel, and UKIDSS observations to study one such cloud, G148.24+00.41, and find that the central area of the cloud is actively forming protostars and is moderately fractal with a Q-value of ∼ 0.66.
Understanding the relative importance of magnetic field, gravity, and turbulence in star formation at the hub of the giant molecular cloud G148.24+00.41
Vineet Rawat,Manash R. Samal,Chakali Eswaraiah,Jia-wei Wang,D. Elia,Sandhyarani Panigrahy,Annie Zavagno,R. K. Yadav,D. L. Walker,J. Jose,D. K. Ojha,C. P. Zhang,S. R. Laboratory,Gujarat,India,Indian Institute of Technology Gandhinagar,Indian Institute of Science Education,Research Tirupati,A. S. I. O. Astronomy,Astrophysics,Taipei,Taiwan,Istituto di Astrofisica e Planetologia Spaziali,-INAF,Italy,Aix-Marseille Universite,Cnrs,Cnes,Lam,France,I. France,Paris,National Astronomical Research Institute of Thailand,Thailand,J. B. C. F. Astrophysics,Department of Physics,Astronomy,U Manchester,Uk,D. Astronomy,T. I. O. F. Research,Mumbai,National Astronomical Observatories,Chinese Academy of Sciences,Beijing,P. R. China,Guizhou Radio Astronomical Observatory,Guizhou University,Guiyang +48 more
TL;DR: High-resolution dust polarization observations reveal the dominant role of gravity over magnetic fields and turbulence in star formation at the hub of G148.24+00.41.
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Star formation efficiency and scaling relations in parsec-scale cluster-forming clumps
Vineet Rawat,Manash R. Samal,Annie Zavagno,Sami Dib,Davide Elia,J. Jose,D. K. Ojha,K. P. R. Laboratory,Ahmedabad.,India,Indian Institute of Technology Gandhinagar,A. Univ,Cnrs,Cnes,Lam Marseille,France,I. France,M. F. Astronomie,Heidelberg,Germany,I. D. A. E. P. Spaziali,-INAF,Roma,Italy,Indian Institute of Science Education,Research Tirupati,D. O. Astronomy,Astrophysics,T. I. O. F. Research,Mumbai +29 more