Results 131 to 140 of about 4,353 (222)

Experimental evidence for granular shear-flow instability in the Epstein regime. [PDF]

open access: yesCommun Phys
Capelo HL   +9 more
europepmc   +1 more source

IUE and IRAS observations of luminous M stars with varying gas-to dust ratios

open access: yes, 1986
Circumstellar gas and dust surrounding M giants and supergiants show luminous M stars to split into two distinct classes. Stars with a high gas to dust ratio all show chromospheric Ca II, H, and K emission. Stars with a high dust to gas ratio do not show
Carpenter, K. G.   +2 more
core  

Gas-phase synthesis of the bicyclic silicon tricarbide molecule (c-SiC<sub>3</sub>) as a precursor to silicon carbide nanoparticles in space. [PDF]

open access: yesChem Sci
Goettl SJ   +10 more
europepmc   +1 more source

A radio-detected type Ia supernova with helium-rich circumstellar material. [PDF]

open access: yesNature, 2023
Kool EC   +36 more
europepmc   +1 more source

The influence of grain growth in circumstellar dust envelopes on observed colors and polarization of some eruptive stars

open access: yes, 1989
R CrB stars are classical examples of stars where dust envelope formation takes place. Dust envelope formation was detected around the Kuwano-Honda object (PU Vul) in 1980 to 1981 when the star's brightness fell to 8(sup m).
Efimov, Yu. S.
core  

The circumstellar dust of MU Cephei

open access: yesThe Astrophysical Journal, 1983
C. Rogers, P. G. Martin, D. R. Crabtree
openaire   +1 more source

Infrared emission towards SN 1987A, 11 years after outburst: Properties of the circumstellar dust

open access: yes, 2002
Detailed models are presented for the late epoch mid infrared (MIR) emission from collisionally heated grains in the shocked circumstellar gas around SN 1987A.
Tuffs, R., Völk, H., Fischera, J.
core  

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