* S. Chandrasekhar, Newton ’ s Principia for the common reader ( New York: Oxford University Press, 1995 ).

#* Anoushka Shankar: sitar, conductor / Sukanya Shankar: vocal-shloka / M. Balanchandar: mridangam / Rajendara Prasanna: shahnai Vishwa Mohan Bhatt: mohan vina / Tanmoy Bose: tabla, dholak / Chandrasekhar and Balu Raghuraman: violins / Eric Clapton: guitar / Pedro Eustache: winds / Sunil Gupta: flute / Anuradha Krishamurthi and O. S.

* Chandrasekhar, S. ( 1958 ).

* Saatchi ( film ), a 1983 Tamil film directed by S. A. Chandrasekhar

* K. Chandrasekhar, J. S. R. L. Narayana Moorty, Stopped In Our Tracks: Stories of UG in India.

The araimudi is also known as the " Genital shield " and an araimudi was mentioned in the " Guide to the principal exhibits in the Government Museum, Pudukkottai ", by M. S. Chandrasekhar, published in 1966 as being displayed in an exhibit in the Madras Government Museum.

He finished as his team's leading wicket taker ( second in the series to Indian leg spinner B. S. Chandrasekhar ) with 19 wickets at less than 20 runs each and helped his team to a 2-1 victory.

* S. Chandrasekhar, M. Kac, R. Smoluchowski, " Marian Smoluchowski-his life and scientific work ", ed.

Meena, all time favorite actress of actor vijay was rumored to have been roped into a movie name " Sattam our iruttarai " which was a remake of the movie under the same name by his father and director, S. A. Chandrasekhar.

Considered amongst the top echelon of leg-spinners, Chandrasekhar along with E. A. S.

# REDIRECT B. S. Chandrasekhar

Shankar began his career as an assistant to film directors like S. A. Chandrasekhar and Pavithran.

His first break in Hindi films was as an assistant director to S. A. Chandrasekhar in Jai Shiv Shankar produced by Rajesh Kanna.

* Chandrasekhar, S. ( 1950 ).

# REDIRECT B. S. Chandrasekhar

Xanthopoulos with S. Chandrasekhar ( Nobel of Physics 1983 )

Kulkarni made her debut through the Tamil film Nanbargal which was directed by S. A. Chandrasekhar.

# REDIRECT B. S. Chandrasekhar

# REDIRECT B. S. Chandrasekhar

* Chandrasekhar, S .: Ellipsoidal Figures of Equilibrium, Yale Univ.

* 1961 – V. B. Chandrasekhar, Indian cricketer

In 1931, Subrahmanyan Chandrasekhar calculated, using special relativity, that a non-rotating body of electron-degenerate matter above a certain limiting mass ( now called the Chandrasekhar limit at 1. 4 solar masses ) has no stable solutions.

They were partly correct: a white dwarf slightly more massive than the Chandrasekhar limit will collapse into a neutron star, which is itself stable because of the Pauli exclusion principle.

But in 1939, Robert Oppenheimer and others predicted that neutron stars above approximately three solar masses ( the Tolman – Oppenheimer – Volkoff limit ) would collapse into black holes for the reasons presented by Chandrasekhar, and concluded that no law of physics was likely to intervene and stop at least some stars from collapsing to black holes.

The Chandrasekhar limit () is the maximum mass of a stable white dwarf star.

It was named after Subrahmanyan Chandrasekhar, the Indian-American astrophysicist who predicted it in 1930.

The Chandrasekhar limit is the mass above which electron degeneracy pressure in the star's core is insufficient to balance the star's own gravitational self-attraction.

This is the Chandrasekhar limit.

Chandrasekhar < sup >, eq.

where the Indian physicist Subrahmanyan Chandrasekhar worked on the calculation of the statistics of a degenerate Fermi gas.

Chandrasekhar reviews this work in his Nobel Prize lecture.

Although Bohr, Fowler, Pauli, and other physicists agreed with Chandrasekhar's analysis, at the time, owing to Eddington's status, they were unwilling to publicly support Chandrasekhar .< sup >, pp. 110 – 111 </ sup > Through the rest of his life, Eddington held to his position in his writings, including his work on his fundamental theory.

The drama associated with this disagreement is one of the main themes of Empire of the Stars, Arthur I. Miller's biography of Chandrasekhar.

If a main-sequence star is not too massive ( less than approximately 8 solar masses ), it will eventually shed enough mass to form a white dwarf having mass below the Chandrasekhar limit, which will consist of the former core of the star.

It has been inferred that as the white dwarf's mass approaches the Chandrasekhar limit, its central density increases, and, as a result of compressional heating, its temperature also increases.

Since the observation of the Champagne Supernova in 2003, more very bright type Ia supernovae are thought to have originated by white dwarfs whose masses exceeded the Chandrasekhar limit.

The limit of neutron degeneracy pressure, analogous to the Chandrasekhar limit, is known as the Tolman – Oppenheimer – Volkoff limit.

* On Stars, Their Evolution and Their Stability, Nobel Prize lecture, Subrahmanyan Chandrasekhar, December 8, 1983.

* White dwarf stars and the Chandrasekhar limit, Masters ' thesis, Dave Gentile, DePaul University, 1995.

After a talk by Chandrasekhar on the limit in 1935, he replied:

In the so-called Type Ia supernovae, gases falling onto a white dwarf raise its mass until it nears a critical level, the Chandrasekhar limit, resulting in an explosion ; in Type Ib / c and Type II supernovae, the progenitor star is a massive star which runs out of fuel to power its nuclear fusion reactions and collapses in on itself, reaching such phenomenal temperatures that it explodes.

Previous to Light's landmark study, which was based on work by Chandrasekhar, investigators unsuccessfully attempted to use other criteria, such as specific gravity, pH, and protein content of the fluid, to differentiate between transudates and exudates.

In decades past, legendary spin bowlers — most notably the Indian spin quartet of the 1960s and 1970s, consisting of left-armer Bedi, offspinners Prasanna and Venkataraghavan, and legspinner Chandrasekhar — routinely toyed with visiting teams to plot dramatic victories for India in home test matches, particularly on turning pitches in hot, humid conditions at Eden Gardens in Kolkata ( then known as Calcutta ) and Chepauk in Chennai ( then known as Madras ).

As examples, the virial theorem may be used to estimate stellar temperatures or the Chandrasekhar limit on the mass of white dwarf stars.

Congratulating Hambardzumyan on his 80th birthday, Subrahmanyan Chandrasekhar who won the Nobel Prize for Physics in 1983, wrote, " The only other astronomer of this century who compares with Academician Hambardzumyan in his consistency and devotion to astronomy is Professor Jan Oort ; but they would appear to be dissimilar in every other way.

They collaborate on the screen-writing, acting and productions of their films, with Chandrasekhar and Heffernan being the primary directors.

* 1970: Chandrasekhar pushes on to 5 / 2 post-Newtonian order,

Sri H R Chandrasekhar, a retired Canara Bank official, is an avid follower and a lecturer on Mankuthimmana Kagga.

Sripati Chandrasekhar ( 22 Nov. 1918, Rajahmundry-14 June 2001 San Diego, Calif .) was a well-known Indian demographer, economist, sociologist, and scholar who as published extensively on demographics, especially related to India.

During this time, he collaborated with Subrahmanyan Chandrasekhar on colliding plane waves.

Ray guest starred in USA Network series Psych, which was directed by Jay Chandrasekhar, which aired on 30 November 2009 and also appeared in a guest role of a reporter, Dominique Ball, in the recent Woody Harrelson movie Defendor.

He finished his doctoral thesis on Astronomy and Astrophysics at University of Chicago under Subrahmanyan Chandrasekhar in 1963.

* 1970: Chandrasekhar pushes on to 5 / 2 post-Newtonian order,