durbin-e bâlon-bord, teleskop-e ~
Fr.: télescope porté par ballon
A remotely guided or automatic telescope carried to high altitudes by a balloon.
→ balloon astronomy; borne "a past participle of bear," from O.E. beran "bear, bring, wear," from P.Gmc. *beranan (O.H.G. beran, Goth. bairan "to carry"), from PIE root *bher-; "to carry;" compare with Av./O.Pers. bar- "to bear, carry," bareθre "to bear (infinitive)," bareθri "a female that bears (children), a mother," Mod.Pers. bordan "to carry," Skt. bharati "he carries," Gk. pherein, L. fero "to carry." → telescope.
→ balloon astronomy. Bord in bâlon-bord "borne, carried," from Mod.Pers. bordan "to bear, carry," as explained above. Durbin, → telescope.
Brought forth by → birth. Past participle of bear. → born-again AGB star.
M.E., from O.E. boren, p.p. of beran "to bear, bring, wear", from P.Gmc. *beranan (O.H.G. beran, Goth. bairan "to carry"), from PIE root *bher- "to bear; to carry" (cf. Av./O.Pers. bar- "to bear, carry," bareθre "to bear (infinitive)," bareθri "a female that bears (children), a mother," Mod.Pers. bordan "to carry," bâr "charge, load", bârdâr "pregnant," Skt. bharati "he carries," Gk. pherein).
Zâdé "born," p.p. of zâdan "give birth" (Av. zan- "to bear, give birth to a child, be born," infinitive zizâite, zâta- "born," cf. Skt. janati "begets, bears," Gk. gignesthai "to become, happen," L. gignere "to beget," gnasci "to be born," PIE base *gen- "to give birth, beget").
born-again AGB star
setâre-ye AGB-ye bâzzâdé
Fr.: étoile AGB recyclée
A → post-AGB star that undergoes a last → thermal pulse when it is already on the → white dwarf → cooling track. The thermal pulse will expand the hot central star, whereby hydrogen will be ingested into the → helium burning shell. This will temporarily return the star to the → AGB phase it has previously left.
→ born; → again; → asymptotic giant branch; → star.
born-again planetary nebula
miq-e sayâreyi-ye bâzzâd
Fr.: nébuleuse planétaire recyclée
A → planetary nebula which is thought to have experienced a → very late thermal pulse (VLTP) when the central star (→ CSPN) was on the → white dwarf cooling track. The VLTP event occurs when the thermonuclear → hydrogen shell burning has built up a → shell of helium with the critical mass to ignite its → fusion into carbon and oxygen (→ helium shell burning). Since the → white dwarf envelope is shallow, the increase of pressure from this last helium shell flash leads to the ejection of newly processed material inside the old planetary nebula, leaving the stellar core intact. As the stellar envelope expands, its → effective temperature decreases and the star goes back to the → asymptotic giant branch (AGB) region in the → H-R diagram. The subsequent stellar evolution is fast and will return the star back to the → Post-AGB track in the H-R diagram: the envelope of the star contracts, its effective temperature and ionizing photon flux increase, and a new fast stellar wind develops (see, e.g. J. A. Toalá et al. 2015, ApJ 799, 67).
Fr.: dernier né
Last in order of birth; youngest.
Demâzâ, from Lori, Laki demâzâ, from demâ "last, end, back," related to dom, → tail, + zâ contraction of zâd, → born.