Wojciech Krzemiński

Wojciech Krzemiński
Wojciech Krzemiński
	NCAC in Warsaw ; and the Carnegie Institution Observatories
Patrons	Polish Academy of Sciences

Wojciech Krzemiński (20 May 1933 – 5 August 2017) was a Polish

Nicolaus Copernicus Astronomical Center of Polish Academy of Sciences. He worked many years for the Carnegie Institution for Science

Observatories.

Biography

Wojciech Krzemiński was a student of professors

Bohdan Paczyński and Józef Smak. In the 1980s he received an offer to take over as administrator or "resident astronomer" of Las Campanas, position which he held for 16 years. He lived many years in La Serena in Chile and returned to Poland in 2011.^[1]

Bohdan Paczynski

Scientific achievements

Wojciech Krzemiński was one of the first observers, who in the 1960s demonstrated the dual nature of

inner Lagrange point of less massive component of binary star

system.

Also in the 1960s, he performed accurate measurements of the brightness of

dwarf novae like U Geminorum

, discovered on 4 December 1961. The marked eclipse of U Geminorum repeated with a period of 4 hours 14 minutes and 45 seconds for the first time clearly demonstrating that we are dealing with a double system.

In his original model Krzemiński interpreted the observed changes in the light curve as a consequence of the uneven luminous surface of a white dwarf. Soon, however, it turned out that in the case of U Geminorum it is not a white dwarf that is obscured. Correct model of the system was introduced by Józef Smak, which is for a binary system containing a white dwarf and filling Roche surface of star in main sequence, made the accretion disc and the so-called "hot spot" that is the place where accreting matter collides with the disc. It is the emergence of "hot spots" behind the disc and its eclipse by the secondary component that was responsible for the unusual appearance of the light curve of U Geminorum.^[2]

In 1964, Krzemiński and Robert Kraft discovered that the star WZ Sagittae (WZ Sge) is a cataclysmic new dwarf of circulation one hour and 22 minutes. This system is interesting in that it erupts approximately every 11,000 days, increasing in brightness by over a thousand. The outbreak is most likely caused by the instability of the accretion disc, which causes periodic falling on the surface of the white dwarf significantly larger portion of matter.

Krzemiński also discovered the optical companion of X-ray pulsar Centaurus X-3, which was named Krzemiński's Star in his honor.

He was also one of the first astronomers who correctly interpreted the nature of polar stars like AM Herculis.

Membership in organizations

He was a member of Polish Astronomical Society, including in the years 1951–1961 when he was secretary of the board.

References

^ "The side of the world – Ep. 11 Wojciech Krzemiński and Andrzej Udalski". www.TELE – program.pl : TVP Polonia. 2011-07-11. Retrieved 2011-11-07.^{[dead link]}
^ "Konferencja "50 lat zaćmień U Geminorum"" [Conference "50 years of eclipses U Geminorum"] (in Polish). PAP-Science in Poland. 2011-10-25. Archived from the original on 2017-09-19. Retrieved 2011-11-07.

[1] "The side of the world – Ep. 11 Wojciech Krzemiński and Andrzej Udalski". www.TELE – program.pl : TVP Polonia. 2011-07-11. Retrieved 2011-11-07.^{[dead link]}

[2] "Konferencja "50 lat zaćmień U Geminorum"" [Conference "50 years of eclipses U Geminorum"] (in Polish). PAP-Science in Poland. 2011-10-25. Archived from the original on 2017-09-19. Retrieved 2011-11-07.

[1]

[2]

Authority control databases
International	VIAF
National	Poland