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PROBLEMS IN GASEOUS HYDRODYNAMICS MICHAŁ RÓŻYCZKA NICOLAUS COPERNICUS ASTRONOMICAL CENTER WARSAW, POLAND. PLANETARY NEBULAE AS ASTRONOMICAL TOOLS GDAŃSK, 28.06.2005. TALK PLAN. THE TEMPLATE: PIECES OF THE PUZZLE:. THE GENERIC NEBULA ...AND SOME EXTRA FLAVOURS.
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PROBLEMS IN GASEOUS HYDRODYNAMICS MICHAŁ RÓŻYCZKA NICOLAUS COPERNICUS ASTRONOMICAL CENTER WARSAW, POLAND PLANETARY NEBULAE AS ASTRONOMICAL TOOLS GDAŃSK, 28.06.2005
TALK PLAN • THE TEMPLATE: • PIECES OF THE PUZZLE: • THE GENERIC NEBULA • ...AND SOME EXTRA FLAVOURS • INTRODUCTION: 1-D HYDRO • 2-D WORLD • 3-D WORLD • SMALL-SCALE FEATURES • MHD
THE TEMPLATE THE GENERIC NEBULA
THE GENERIC NEBULA ... VERY HOT GAS („HOT CAVITY”) A BIG MESS INSIDE ORDERLY RINGS THE GENERIC NEBULA SPHERICAL HALO
THE TEMPLATE EXTRA FLAVOURS
TADPOLES SOME EXTRA FLAVOURS HOT CAVITY
WAVES BIPOLAR LOBES SOME EXTRA FLAVOURS
POINT SYMMETRY SOME EXTRA FLAVOURS
MULTIPOLAR OUTFLOWS SOME EXTRA FLAVOURS
FLIERS SOME EXTRA FLAVOURS
ANSAE SOME EXTRA FLAVOURS
JETS DISKS SOME EXTRA FLAVOURS
BRETS BIPOLAR ROTATING EPISODIC JETS SOME EXTRA FLAVOURS
HUBBLE FLOW (v ~ R) BIPOLAR LOBES SOME EXTRA FLAVOURS
PIECES OF THE PUZZLE INTRODUCTION: 1-D HYDRO
contact surface contact surface contact surface reverse shock reverse shock reverse shock forward shock forward shock forward shock free wind 1 free wind 1 free wind 1 shocked wind 1 shocked wind 1 shocked wind 1 shocked wind 2 shocked wind 2 shocked wind 2 free wind 2 free wind 2 free wind 2 CONTACT SURFACE FRAME FREE WIND 2 FRAME (=AMBIENT MEDIUM FRAME) CONTACT SURFACE FRAME INTRODUCTION: 1-D HYDRO
INTRODUCTION: 1-D HYDRO forward shock reverse shock contact surface free fast wind shocked fast wind shocked AGB wind free AGB wind
. . INTRODUCTION: 1-D HYDRO Balick, B. & Frank, A. 2002; ARAA 40, 439
. . INTRODUCTION: 1-D HYDRO Balick, B. & Frank, A. 2002; ARAA 40, 439
FS CS RS INTRODUCTION: 1-D HYDRO
PIECES OF THE PUZZLE 2-D WORLD
FOR SMALL DEPARTURES FROM SPHERICAL SYMMETRY: Icke V. 1988; A&A 202, 177 2-D WORLD: BASICS ROTATION BINARY INTERACTIONS MAGNETIC FIELDS
2-D WORLD: BASICS forward shock reverse shock shocked AGB wind free fast wind contact surface shocked fast wind free AGB wind
2-D WORLD: OBLIQUE SHOCKS OBLIQUE SHOCK shocked wind 2 free wind 2 SHOCK FRAME
. . Mslow=10-5 M/yr Mfast =10-7 M/yr 2-D WORLD: SHAPING - BIPOLARS q = 0.1 veq Vpl/ Veq = 3 vpl Garcia-Segura,G. et al. 1999; ApJ 517, p.767
Norman, M., Smarr, L., Smith, M., & Wilson, J. 1981; ApJ 247, 52 2-D WORLD: COLLIMATION, JETS-I Blandford, R. & Rees, M. 1974; MNRAS 169, 395
. Mw = 10-7 M/yr Vw = 200 km/s adiabatic 3 FS CS RS 2-D WORLD: COLLIMATION, JETS-I Frank, A. & Mellema, G. 1996; ApJ 472, 684
. Mw = 10-7 M/yr Vw = 200 km/s adiabatic q = 70 2-D WORLD: COLLIMATION, JETS-I Frank, A. & Mellema, G. 1996; ApJ 472, 684
2-D WORLD: COLLIMATION, JETS-I Frank, A. & Mellema, G. 1996; ApJ 472, 684
forward shock contact surface reverse shock T 2-D WORLD: COLLIMATION, JETS-II
PIECES OF THE PUZZLE 3-D WORLD
RG star: M*=1M; R*=0.7 AU secondary: M*=0.6 M RG wind: 10-6 M/yr fast wind: 10-8 M/yr; 103 km/s a = 2.4 AU a = 12.6 AU 3-D WORLD: BINARY, DENSE WIND SHAPING Gawryszczak, A., Mikołajewska, J. & Różyczka, M. 2002; A&A 385, 205
3-D WORLD: BINARY, DENSE WIND SHAPING Gawryszczak, A., Mikołajewska, J. & Różyczka, M. 2002; A&A 385, 205
RW Hya RED GIANT: M=1.6M, R=1013 cm, M=10-7 M/yr WHITE DWARF: M=0.48 M, a=21013 cm . 3-D WORLD: BINARY, DISK FORMATION Courtesy: Doris Folini & Rolf Walder http://www.astro.phys.ethz.ch/staff/walder/
SYMBIOTIC BINARY COOL STAR: M=1.4M, R=1013 cm, M=310-8 M/yr HOT STAR: M=0.6 M, a=31013 cm, M=410-9 M/yr . . 3-D WORLD: BINARY, DENSE WIND SHAPING HIGH LOW Courtesy: Doris Folini & Rolf Walder http://www.astro.phys.ethz.ch/staff/walder/
3-D WORLD: BINARY, COMMON ENVELOPE EVOLUTION red giant: 1 Mwith a 0.45 M core companion: 0.35 M Movies by Eric Sandquist; http://mintaka.sdsu.edu/faculty/erics/web/
3-D WORLD: BINARY, COMMON ENVELOPE EVOLUTION Eric Sandquist; http://mintaka.sdsu.edu/faculty/erics/web/
170 days 1130 days 2310 days 3250 days 3-D WORLD: BINARY, COMMON ENVELOPE EVOLUTION AGB star core 0.56 M envelope 0.69 M radius 1.85 AU companion mass 0.1 M timesscale 9 yr mass lost 4 % AGB star core 0.56 M envelope 0.69 M radius 1.85 AU companion mass 0.1 M synchronous timesscale 9 yr mass lost 25 % AGB star core 0.60 M envelope 0.44 M radius 3.00 AU companion mass 0.1 M timesscale 18 yr mass lost 84 % De Marco, O. Et al. 2003; RevMexAA S.Conf. 18,24
PIECES OF THE PUZZLE SMALL-SCALE FEATURES
~T-0.7 SMALL-SCALE FEATURES: COOLING INSTABILITY Gaetz,T. & Salpeter, E. 1983; ApJS 52, 155
SMALL-SCALE FEATURES: COOLING INSTABILITY; R-T INSTABILITY Movie: courtesy Doris Folini & Rolf Walder http://www.astro.phys.ethz.ch/staff/walder/
density schematic: denser fluid g lighter fluid SMALL-SCALE FEATURES: RAYLEIGH-TAYLOR INSTABILITY density range: 0.5 – 2.5 g/cm3 simulation time:3.1 sec Movie: courtesy ASC / Alliances Center for Astrophysical Thermonuclear Flashes http://flash.uchicago.edu/website/research/gallery/home.py
nonisotropic ram pressure isotropic thermal pressure SMALL-SCALE FEATURES: THIN SHELL INSTABILITY I Vishniac, E. 1983; ApJ 274, 152
free AGB wind forward shock shocked AGB wind shocked fast wind SMALL-SCALE FEATURES: THIN SHELL INSTABILITY I
SMALL-SCALE FEATURES: THIN SHELL INSTABILITY II nonisotropic ram pressure nonisotropic ram pressure Vishniac, E. 1994; ApJ 428, 186
SMALL-SCALE FEATURES: THIN SHELL INSTABILITY II SPHERICAL SYMMETRY: IONIZATION INSTABILITIES (?) SPHERICAL SYMMETRY: RAYLEIGH-TAYLOR INSTABILITY AXIAL SYMMETRY: KELVIN-HELMHOLTZ INSTABILITY Movie: courtesy Doris Folini & Rolf Walder http://www.astro.phys.ethz.ch/staff/walder/
SMALL-SCALE FEATURES: THIN SHELL INSTABILITY II John Blondin http://wonka.physics.ncsu.edu/~blondin/aas196/page33.html