EC
Eswaraiah Chakali
Also known as: Eswaraiah C
Indian Institute of Science Education and Research (IISER) Mohali, Indian Institute of Science Education and Research Tirupati, Sri Venkateswara University
Employment
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Indian Institute of Science Education and Research (IISER) Mohali Assistant Professor2025 - Present
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Indian Institute of Science Education and Research Tirupati Ramanujan Fellow2021 - Present
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National Astronomical Observatories Chinese Academy of Sciences FAST Fellow2018 - 2021
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Indian Institute of Astrophysics Visiting Scientist2018 - 2018
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National Tsing-Hua University Department of Physics Postdoc2015 - 2018
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National Central University (NCU) Postdoc2013 - 2015
Education
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Aryabhatta Research Institute of Observational Sciences (ARIES) / Kumaun University PhD2006 - 2013
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Sri Venkateswara University MSc2004 - 2006
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Sri Venkateswara University BSc2002 - 2006
Projects & Funding
Projects & funding information is unavailable.
Publications (55)
- Evidence for the gravity-driven and magnetically-regularized gas flows feeding the massive protostellar cluster in Cep A Save
- Magnetic field topology and star formation in the Cepheus B filamentary cloud under external feedback Save
- VolDen: A tool to extract number density from the column density of filamentary molecular clouds Save
- 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 Save
- Galactic ‘Snake’ IRDC G11.11−0.12: a site of multiple hub–filament systems and colliding filamentary clouds Save
- Correction to: Revealing the dust grain polarization properties as a function of extinction and distance towards NGC 1893 Save
- Role of magnetic fields in the fragmentation of the Taurus B213 filament into Sun-type star-forming cores Save
- Star-forming site RAFGL 5085: Is a perfect candidate of hub-filament system? Save
- Revealing the dust grain polarization properties as a function of extinction and distance towards NGC 1893 Save
- The JCMT BISTRO Survey: Revealing the Diverse Magnetic Field Morphologies in Taurus Dense Cores with Sensitive Submillimeter Polarimetry Save