Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Maji, Moupiya"'
Autor:
Maji, Moupiya, More, Surhud, Sule, Aniket, Balasubramanya, Vishaak, Bhandari, Ankit, Chand, Hum, Chavan, Kshitij, Dasgupta, Avik, De, Anindya, Gangopadhyay, Jayant, Gulati, Mamta, Hasan, Priya, Ishtiyaq, Syed, Madani, Meraj, Misra, Kuntal, N, Amoghavarsha, Oberoi, Divya, Pattnaik, Subhendu, Patwardhan, Mayuri, Ramanujam, Niruj Mohan, Ranadive, Pritesh, Sawant, Disha, Sharma, Paryag, Sharma, Twinkle, Shetye, Sai, Singhal, Akshat, Srivastava, Ajit M., Sudan, Madhu, Syed, Mumtaz, Vikranth, Pulamathi, Yadav, Virendra
We present the results of a nation-wide baseline survey, conducted by us, for the status of Astronomy education among secondary school students in India. The survey was administered in 10 different languages to over 2000 students from diverse backgro
Externí odkaz:
http://arxiv.org/abs/2406.12308
Autor:
Rodruck, Michael, Charlton, Jane, Borthakur, Sanchayeeta, Chitre, Aparna, Durrell, Patrick R., Elmegreen, Debra, English, Jayanne, Gallagher, Sarah C., Gronwall, Caryl, Knierman, Karen, Konstantopoulos, Iraklis, Li, Yuexing, Maji, Moupiya, Mullan, Brendan, Trancho, Gelys, Vacca, William
We present results of a Hubble Space Telescope (HST) UBVI-band study of star clusters in tidal tails, using new WFC3 and ACS imaging to complement existing WFPC2 data. We survey 12 tidal tails across seven merging systems, deriving ages and masses fo
Externí odkaz:
http://arxiv.org/abs/2309.10267
Autor:
Maji, Moupiya, Verhamme, Anne, Rosdahl, Joakim, Garel, Thibault, Blaizot, Jeremy, Mauerhofer, Valentin, Pittavino, Marta, Feser, Maria-Pia Victoria, Chuniaud, Mathieu, Kimm, Taysun, Katz, Harley, Haehnelt, Martin
Publikováno v:
A&A 663, A66 (2022)
The primary difficulty in understanding the sources and processes that powered cosmic reionization is that it is not possible to directly probe the ionizing Lyman Continuum (LyC) radiation at that epoch as those photons have been absorbed by the inte
Externí odkaz:
http://arxiv.org/abs/2204.02440
Autor:
Zhu, Qirong, Li, Yuexing, Li, Yiting, Maji, Moupiya, Yajima, Hidenobu, Schneider, Raffaella, Hernquist, Lars
Supermassive black holes (SMBHs) of $\sim 10^9\, M_\odot$ are generally believed to be the central engines of the luminous quasars observed at $z\gtrsim6$, but their astrophysical origin remains elusive. The $z\gtrsim$ quasars reside in rare density
Externí odkaz:
http://arxiv.org/abs/2012.01458
ART$^2$ is a 3D multi-wavelength Monte Carlo radiative transfer (RT) code that couples continuum and emission lines to track the propagation of photons and their interactions with the interstellar medium (ISM). The previous version of ART$^2$, which
Externí odkaz:
http://arxiv.org/abs/2001.11146
Autor:
Maji, Moupiya
Pattern speed is an important parameter of the density wave theory for spiral galaxies. In this thesis we have determined the pattern speed for warped galaxies (flat galaxies being a special case of this generalization) using the observable data of t
Externí odkaz:
http://etd.iisc.ernet.in/handle/2005/2456
http://etd.ncsi.iisc.ernet.in/abstracts/3171/G25444-Abs.pdf
http://etd.ncsi.iisc.ernet.in/abstracts/3171/G25444-Abs.pdf
It has been suggested that the satellite galaxies of the Milky Way reside in a highly-flattened, kinematically-coherent plane called Disk of Satellites (DoS). The origin of the DoS, however, has been hotly debated, and a number of conflicting claims
Externí odkaz:
http://arxiv.org/abs/1702.00497
Publikováno v:
The Astrophysical Journal, Volume 843, Number 1, Pages 62 (2017)
The "Disk of satellites" (DoS) around Milky Way is a highly debated topic with conflicting interpretations of observations and their theoretical models. We perform a comprehensive analysis of all dwarfs detected in the Milky Way and find that the DoS
Externí odkaz:
http://arxiv.org/abs/1702.00485
Observations of globular clusters show that they have universal lognormal mass functions with a characteristic peak at $\sim 2\times 10^{5}\, {\rm{M_{\odot}}}$, but the origin of this peaked distribution is highly debated. Here we investigate the for
Externí odkaz:
http://arxiv.org/abs/1606.07091
Autor:
Zhu, Qirong, Marinacci, Federico, Maji, Moupiya, Li, Yuexing, Springel, Volker, Hernquist, Lars
We study the impact of baryons on the distribution of dark matter in a Milky Way-size halo by comparing a high-resolution, moving-mesh cosmological simulation with its dark matter-only counterpart. We identify three main processes related to baryons
Externí odkaz:
http://arxiv.org/abs/1506.05537