- Stellar, planetary, and galactic studies
- Astronomy and Astrophysical Research
- Adaptive optics and wavefront sensing
- Gamma-ray bursts and supernovae
- Criminal Justice and Corrections Analysis
- Galaxies: Formation, Evolution, Phenomena
- Diverse scientific research topics
- Electrical and Electromagnetic Research
- Radioactive Decay and Measurement Techniques
- Phase Equilibria and Thermodynamics
- Astrophysics and Star Formation Studies
- Advanced Mathematical Theories and Applications
- Radiation Detection and Scintillator Technologies
Arizona State University
2021-2024
Abstract We present the discovery of a low-redshift damped Ly α (DLA) system in spectrum background starburst galaxy SDSS J111323.88+293039.3 ( z = 0.17514). The DLA is at an impact parameter ρ 36 kpc from star-forming galaxy, J111324.08+293051.2 0.17077). measure H i column density N (H ) 3.47 × 10 20 cm −2 along with multiple low-ionization species such as , ii Si C and iii . also make estimate covering fraction to be 0.883, giving us limiting size A ≥ 3.3 2 Assuming uniform over entire...
As a part of the Deciphering Interplay between Interstellar medium, Stars, and Circumgalactic medium (DIISC) survey, we investigate indirect evidence gas inflow into disk galaxy NGC 99. We combine optical spectra from Binospec spectrograph on MMT telescope with imaging data Vatican Advanced Technology Telescope, radio HI 21 cm emission images NSF Karl G. Jansky's Very Large Array, UV spectroscopy Cosmic Origins Spectrograph Hubble Space Telescope. measure lines (H$\alpha$, H$\beta$, [O...
Abstract As a part of the Deciphering Interplay between Interstellar medium, Stars, and Circumgalactic medium (DIISC) survey, we investigate indirect evidence gas inflow into disk galaxy NGC 99 . We combine optical spectra from Binospec spectrograph on MMT telescope with imaging data Vatican Advanced Technology Telescope, radio H i 21 cm emission images NSF Karl G. Jansky’s Very Large Array, UV spectroscopy Cosmic Origins Spectrograph Hubble Space Telescope. measure lines (H α , β [O iii ] λ...