Zobrazeno 1 - 10
of 3 822
pro vyhledávání: '"Ghosh, S. K."'
Autor:
George, Koshy, Poggianti, B. M., Omizzolo, A., Vulcani, B., Côté, P., Postma, J., Smith, R., Jaffe, Y. L., Gullieuszik, M., Moretti, A., Subramaniam, A., Sreekumar, P., Ghosh, S. K., Tandon, S. N., Hutchings, J. B.
The assembly of galaxy clusters is understood to be a hierarchical process with a continuous accretion of galaxies over time, which increases the cluster size and mass. Late-type galaxies that fall into clusters can undergo ram-pressure stripping, fo
Externí odkaz:
http://arxiv.org/abs/2409.10586
The exceptional physicochemical properties and versatile biological activities of ionic liquids (ILs) have propelled their potential applications in various industries, including pharmaceuticals and green chemistry. However, their widespread use is l
Externí odkaz:
http://arxiv.org/abs/2407.18706
Autor:
Sharma, V. K., Gupta, J., Mitra, J. Bhatt, Srinivasan, H., Sakai, V. García, Ghosh, S. K., Mitra, S.
The bactericidal potency of ionic liquids (ILs) is well-established, yet their precise mechanism of action remains elusive. Here, we show evidence that the bactericidal action of ILs primarily involves permeabilizing the bacterial cell membrane. Our
Externí odkaz:
http://arxiv.org/abs/2404.06739
We present a multiwavelength investigation of the hub-filament system RCW 117 (IRAS 17059-4132), which shows intricate filamentary features in the far-infrared, mapped using Herschel images. We obtain the column density and dust temperature maps for
Externí odkaz:
http://arxiv.org/abs/2311.00477
Publikováno v:
Front. Phys. 11, 1256166 (2023)
The silicide superconductors (Ta, Nb, Zr)OsSi are among the best candidate materials for investigating the interplay of topological order and superconductivity. Here, we investigate in detail the normal-state topological properties of (Ta, Nb, Zr)OsS
Externí odkaz:
http://arxiv.org/abs/2310.04105
Autor:
R, Rakhi, Santhosh, Geethika, Joseph, Prajwel, George, Koshy, Subramanian, Smitha, Kavila, Indulekha, Postma, J., Duc, Pierre-Alain, Côté, Patrick, Cortese, Luca, Ghosh, S. K., Subramaniam, Annapurni, Tandon, Shyam, Hutchings, John, Wesley, P Samuel, Bharadwaj, Aditya, Niroula, Neeran
NGC 5291, an early-type galaxy surrounded by a giant HI ring, is believed to be formed from collision with another galaxy. Several star forming complexes and tidal dwarf galaxies are distributed along the collisional ring which are sites of star form
Externí odkaz:
http://arxiv.org/abs/2304.07244
Autor:
George, Koshy, Poggianti, B. M., Tomičić, Neven, Postma, J., Côté, P., Fritz, J., Ghosh, S. K., Gullieuszik, M., Hutchings, J. B., Moretti, A., Omizzolo, A., Radovich, M., Sreekumar, P., Subramaniam, A., Tandon, S. N., Vulcani, B.
Spiral galaxies undergo strong ram-pressure effects when they fall into the galaxy cluster potential. As a consequence, their gas is stripped to form extended tails within which star formation can happen, giving them the typical jellyfish appearance.
Externí odkaz:
http://arxiv.org/abs/2212.02423
The star-forming activity in the HII region RCW 42 is investigated using multiple wavebands, from near-infrared to radio wavelengths. Located at a distance of 5.8 kpc, this southern region has a bolometric luminosity of 1.8 $\times$ 10$^6$ L$_{\odot}
Externí odkaz:
http://arxiv.org/abs/2207.14040
Globular clusters being old and densely packed serve as ideal laboratories to test stellar evolution theories. Although there is enormous literature on globular clusters in optical bands, studies in the ultraviolet (UV) regime are sparse. In this wor
Externí odkaz:
http://arxiv.org/abs/2205.13839