Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Chanda J Jog"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 511:5878-5896
An $m=1$ lopsided asymmetry is common in disc galaxies. Here, we investigate the excitation of an $m=1$ lopsidedness in host galaxies during minor mergers while choosing a set of 1:10 merger models (with varying orbital configurations, morphology of
Autor:
Chanda J. Jog, Suchira Sarkar
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 499:2523-2533
The vertical density distribution of stars in a galactic disc is traditionally obtained by assuming an isothermal vertical velocity dispersion of stars. Recent observations from SDSS, LAMOST, RAVE, Gaia etc show that this dispersion increases with he
Autor:
Chanda J. Jog, Suchira Sarkar
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 492:628-633
The self-consistent vertical density distribution in a thin, isothermal disc is typically given by a sech^2 law, as shown in the classic work by Spitzer (1942). This is obtained assuming that the radial and vertical motions are decoupled and only the
Autor:
Chanda J. Jog, Narendra Nath Patra
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:4942-4951
We examine the H i total intensity maps of the VLA LITTLE-THINGS galaxies and identify an H i bar in the dwarf irregular galaxy DDO 168 which has a dense and compact dark matter halo that dominates at all radii. This is only the third galaxy found to
Autor:
Suchira Sarkar, Chanda J. Jog
Publikováno v:
Astronomy & Astrophysics. 665:A23
We calculate ab initio the gravitational potential energy per unit area for a gravitationally coupled multi-component galactic disk of stars and gas, which is given as the integration over vertical density distribution, vertical gravitational force,
Autor:
Soumavo Ghosh, Chanda J. Jog
A typical galactic disc has a finite thickness and in addition to stars it also contains a finite amount of interstellar gas. Here, we investigate the physical impact of the finite thickness of a galactic disc on the disc stability against the non-ax
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9697a7ade75c9687aad0b57503c15fd1
The study of gas-dust interactions occurring in the interstellar medium of a galaxy is essential for understanding various physical processes taking place within it. A comparison of such events at different locations corresponding to diverse astrophy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::678c464be79eb1df4263423cc30841ad
Autor:
Chanda J. Jog, Suchira Sarkar
Publikováno v:
Proceedings of the International Astronomical Union. 14:13-15
We study the vertical stellar distribution of the Milky Way thin disk treated as a gravitationally coupled system of stars, HI and H2 gas in the field of dark matter halo, from R = 4 to 22 kpc. We show that the gas and halo gravity mainly constrain t
Autor:
Chanda J. Jog, Suchira Sarkar
Publikováno v:
Astronomy & Astrophysics. 652:C1
Autor:
Soumavo Ghosh, Chanda J. Jog
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 459:4057-4065
In the density wave theory of spiral structure, the grand-design two-armed spiral pattern is taken to rotate rigidly in a galactic disc with a constant, definite pattern speed. The observational measurement of the pattern speed of the spiral arms, th