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Anna N. Żytkow

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Anna N. Żytkow
Born (1947-02-21) 21 February 1947 (age 77)
Poland
NationalityPolish
EducationUniversity of Warsaw
Known forThorne–Żytkow object
Scientific career
FieldsAstrophysics
InstitutionsInstitute of Astronomy, Cambridge of the University of Cambridge

Anna Nikola Żytkow (Polish pronunciation: [ˈanna ˈʐɨtkɔf]; born 21 February 1947) is a Polish astrophysicist working at the Institute of Astronomy of the University of Cambridge.[1][2] Żytkow and Kip Thorne proposed a model for what is called the Thorne–Żytkow object, which is a star within another star. Żytkow in 2014 was part of the team led by Emily M. Levesque which discovered the first candidate for such an object.

Thorne-Żytkow objects

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Working together with Kip Thorne in 1976, Żytkow developed a theoretical model for a new star type, the Thorne–Żytkow object (TŻO),[3] which contains either a neutron star or a black hole core at the center of a stellar envelope. The evolution of such a star occurs rarely and only two processes exist that define the structure and evolution of a TŻO.[4] In the first process a collision between a neutron star and a normal star, either dwarf or giant, must occur in order to merge the two into a single object.[4] This occurrence is rare since stars do not usually collide with each other. This could only happen in a dense cluster of stars. The second possible evolution of a larger TŻO can occur when a star expands into a red supergiant and engulfs its companion neutron star.[4]

A team led by Emily Levesque (University of Colorado at Boulder) and including Anna Żytkow found the first viable TŻO candidate using the 6.5-meter Magellan Clay Telescope at Las Campanas Observatory in 2014,[5] possibly succeeding in a search for these bizarre stars, one that had already spanned some 40 years worth of effort.

Żytkow said upon the discovery: "I am extremely happy that observational confirmation of our theoretical prediction has started to emerge. Since Kip Thorne and I proposed our models of stars with neutron cores, people were not able to disprove our work. If theory is sound, experimental confirmation shows up sooner or later. So it was a matter of identification of a promising group of stars, getting telescope time and proceeding with the project."[6]

Personal life

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Żytkow's career was interrupted by a mountaineering accident that nearly took her life.[7]

Kuiper belt discoveries

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Minor planets discovered: 7 [8]
(8012) 1990 HO3 29 April 1990 list
(8361) 1990 JN1 1 May 1990 list
15810 Arawn 12 May 1994 list
(16684) 1994 JQ1 11 May 1994 list
(48443) 1990 HY5 29 April 1990 list
(58165) 1990 HQ5 29 April 1990 list
(73682) 1990 HU5 29 April 1990 list
all co-discovered with Mike Irwin

In December 1995, Mike Irwin, Scott Tremaine, and Anna N. Żytkow collaborated on the survey of two slow-moving objects, which are probable members of the Kuiper belt. Żytkow and the group followed Edgeworth (1949) and Kuipers (1951) research, which indicates that protoplanetary disks extend beyond Neptune and that the disk material beyond Neptune had not coalesced into planets.[9] This group of planetesimals is now known as the Kuiper belt. Żytkow and the rest of the group members spent most of their time adjusting the focus of the camera and instruments attached to the Isaac Newton Telescope (INT). The group used the Monte Carlo method, which provided multiple simulations in two separate stages. The first stage is the detection rate for images that came from INT as a function of magnitude, which was investigated using artificial images adding to the original frames.[9] The second stage involved examining the detection rate for a series of artificial images from INT that followed the typical slow moving solar system objects (SMO) track.[9] The outcome of this survey was a detection of two new Kuiper belts objects within the area of 0.7 degree sq. to a limiting magnitude mR=23.5.[9]

Publications

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References

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  1. ^ Zimmermann, Mark (1 May 2000). "Soft Outside CrunchyCenter". ZhurnalyWiki. Archived from the original on 28 June 2012. Retrieved 24 July 2011.
  2. ^ "Dr Anna N Żytkow". University of Cambridge. Archived from the original on 26 May 2012. Retrieved 24 July 2011.
  3. ^ Thorne, Kip S.; Żytkow, Anna N. (15 March 1977). "Stars with degenerate neutron cores. I - Structure of equilibrium models". The Astrophysical Journal. 212 (1): 832–858. Bibcode:1977ApJ...212..832T. doi:10.1086/155109. Archived from the original on 10 April 2023 – via NASA/ADS.
  4. ^ a b c Cannon, R.; Eggleton, P.; Zytkow, A.; Podsiadlowski, P. (1992). "The Structure and Evolution of Thorne-Zytkow Objects". The Astrophysical Journal. 386. Institute of Astronomy, Madingley Road, Cambridge, UK: 206. Bibcode:1992ApJ...386..206C. doi:10.1086/171006. Archived from the original on 30 May 2023 – via NASA/ADS.
  5. ^ Levesque, Emily; Massey, Philip; Żytkow, Anna; Morrell, Nidia (30 May 2014). "Discovery of a Thorne-Zytkow object candidate in the Small Magellanic Cloud". Monthly Notices of the Royal Astronomical Society Letters. 1406: L94–L98. arXiv:1406.0001. Bibcode:2014MNRAS.443L..94L. doi:10.1093/mnrasl/slu080. Archived from the original on 28 June 2024 – via Oxford Academic.
  6. ^ "Odd Hybrid Star Discovered 40 Years After Scientists Predicted Its Existence". Science. 9 June 2014. Retrieved 4 February 2019.
  7. ^ Katz, Jonathan I. (2002). The Biggest Bangs: The Mystery of Gamma-ray Bursts, the Most Violent Explosions in the Universe. Oxford University Press. p. 79. ISBN 9780198033332. Retrieved 2 February 2002. Anna Zytkow.
  8. ^ "Minor Planet Discoverers (by number)". Minor Planet Center. 23 May 2016. Retrieved 20 June 2016.
  9. ^ a b c d Żytkow, Anna; Irwin, Mike; Tremaine, Scott (1995). "A Search for Slow-Moving Objects and the Luminosity Function of the Kuiper Belt". The Astronomical Journal. 110. Institute of Astronomy, Madingley Road, Cambridge, United Kingdom: 3082. Bibcode:1995AJ....110.3082I. doi:10.1086/117749.
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