Browsing Theses by Issue Date

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  • Dastidar, Raya (ARIES, Nainital, 2021-08)
    Supernovae are the cosmic fireworks that mark the death of stars, wherein heavy elements are forged and dispersed, leading to the galactic enrichment of the Universe. In core-collapse supernovae, the collapse of the inert ...
  • Singh, Kuldeep (ARIES, Nainital, 2021-08)
    A detailed study of magnetized astrophysical ows has been carried out in the magnetohydrodynamic and special relativistic magneto- hydrodynamic regime. We have considered the thermodynamics of the ow to be described ...
  • Jalan, Priyanka (ARIES, Nainital, 2022-02-26)
    Soon after the discovery of the first quasars, a small decrement in the spectrum of a quasar shortward of its Lyα emission line was measured. Recognizing the decrement was due to the Lyα resonance absorption of radiation ...
  • Sarkar, Shilpa (ARIES, Nainital, 2022-06-02)
    Black holes (BHs) are one of the most exotic objects found in the Universe. They fall into a class of astrophysical objects termed as compact objects. Apart from BHs, neutron stars (NSs) and white dwarfs (WDs) also fall ...
  • Srivastava, Priyanka (ARIES, Nainital, 2022-07)
    Tiny particles in the solid, liquid, or mixed phases and suspended in air are known as atmospheric aerosols (Junge, 1963). Despite being minor constituents of the atmosphere, these particles have a profound influence and ...
  • Arora, Bharti (ARIES, Nainital, 2022-07-04)
    Massive stars (initial mass > 8M⊙) are important objects within a galaxy, impacting their environments via their intense radiation fields as well as dense, supersonic winds and subsequently via supernova explosions. This ...
  • Patel, Ritesh (ARIES, Nainital, 2022-08)
    The solar corona is known to be associated with eruptions of large amount of magnetized plasma into the interplanetary space. In-spite of several years of groundand space-based observations of the solar atmosphere, the ...
  • Jha, Bibhuti Kumar (ARIES, 2022-09)
    The Sun shows a wide range of temporal variations, from a few seconds to decades and even centuries, broadly classi ed into two classes short{term and long{term. The solar dynamo mechanism is believed to be responsible ...
  • Chand, Krishan (ARIES, Nainital, 2022-12)
    A compact region at the centre of a galaxy known as an active galactic nucleus (AGN) generates a significant amount of energy that is not directly due to stars. It is believed that the accretion of materials onto ...
  • Singh, Gaurav (ARIES, Nainital, 2023-02-25)
    We present the multi-wavelength study of the hot stellar population in Galactic Globular clusters (GGCs). The population of interest in GCs is Blue straggler stars (BSSs) and the extreme end of the hor izontal branch ...
  • Sinha, Tirthendu (ARIES, Nainital, 2023-03-25)
    The evolution of pre-main-sequence (PMS) stars involves a set of complex physical processes such as evolution of circumstellar disks, accretion processes, bipolar jets and outflows, evolution of angular momentum etc. Because ...
  • Singh, Sadhana (ARIES, Nainital, 2023-06-11)
    The starlight passing through the interstellar medium becomes linearly polarized due to the differential extinction from the alignment of asymmetric dust grains in the medium. Both macroscopic and microscopic information ...
  • Ghosh, Arpan (ARIES, Nainital, 2023-07-04)
    Episodic accretion in young stellar objects (YSOs) are sudden enhance ment of the accretion rate from the circumstellar disc onto the central pre main sequence (PMS) star. During such episodes of enhanced accretion, it has ...
  • Gupta, Rahul (ARIES, Nainital, 2023-09)
    Gamma-ray bursts (GRBs) are fascinating sources studied in modern astronomy. They are extremely luminous electromagnetic (Lγ,iso ∼ 1048 − 1054 erg/s) explosions in the Universe observed from cosmological distances. These ...
  • Dhiman, Vinit (ARIES, Nainital, 2023-10-10)
    Blazars consisting of BL Lacertae objects (BL Lacs; featureless compsite optical/UV spectra) and flat-spectrum radio quasars (FSRQs; promi nent emission lines in composite optical/UV spectra), are the active galactic ...
  • Aryan, Amar (ARIES, Nainital, 2023-12)
    Core-collapse supernovae (CCSNe) are catastrophic astrophysical phenomena that occur during the last evolutionary stages of massive stars having initial masses ≳ 8 M⊙. These catastrophic events play a pivotal role in ...

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