Revisited mass-loss rates for the nuclei of the planetary nebulae NGC 6210, NGC 6826 and NGC 6543 - The first order moment W1 of subordinate line profiles [PDF]
, 1987 peer reviewedThe authors present the results of numerical calculations for the first order moment W[SUB]1[/SUB] of subordinate P Cygni line profiles as a function of the parameter W[SUB]1[/SUB][SUP]0[/SUP]alphaM>n[SUB]g[/SUB]n[SUB]g[/SUB]n[SUB]g[/SUB]
Surdej, Jean, Hutsemekers, Damien
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Delivery of complex organic compounds from evolved stars to the solar system. [PDF]
Orig Life Evol Biosph, 2011 Kwok S.
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Point-symmetry and the double planetary nebula KJPN 8
, 2002 We present recent results of two topical problems on dynamical evolution of Planetary Nebulae (PNe) where binary nuclei, stellar rotation and magnetic elds play relevant roles. Namely, point-symmetry and multiple, collimated outflows.
Miranda, L.F. +8 more
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ALMA high spatial resolution observations of the dense molecular region of NGC 6302. [PDF]
Astron Astrophys, 2017 Santander-García M +7 more
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X-rays from planetary nebulae: Unveiling wind collisions and binarity
, 2010 Planetary nebulae (PNe), the ionized, ejected envelopes of low- to intermediate-mass stars, are thought to be shaped by a nascent fast wind from the spent core (a future white dwarf) that collides with and sweeps up previously ejected material (red and ...
Montez, Rodolfo
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How much graphene in space? [PDF]
Mon Not R Astron Soc, 2019 Li Q, Li A, Jiang BW.
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The Nuclei of Two Planetary Nebulae [PDF]
Monthly Notices of the Royal Astronomical Society, 1933 openaire +1 more source
A half century of infrared astronomy - A personal recollection of the footprints in Japan. [PDF]
Proc Jpn Acad Ser B Phys Biol Sci, 2019 Okuda H.
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Energetic spectra from semi-implicit particle-in-cell simulations of magnetic reconnection. [PDF]
Sci RepSchoeffler KM +4 more
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The Evolution of Planetary Nebula Nuclei
, 1985 The evolution of planetary nebula nuclei (PNNs) is examined with the aid of the most recent available stellar evolution calculations and new observations of these objects.
Shaw, Richard Allen
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