Results 181 to 190 of about 9,125 (216)

Dynamics of non-self-similar earthquakes illuminated by a controlled fault asperity. [PDF]

Nat Commun
Okubo K, Yamashita F, Fukuyama E.
europepmc   +1 more source

Out-of-Equilibrium Supramolecular Assembly Sustained by Photocatalysis. [PDF]

Angew Chem Int Ed Engl
Pelorosso E, Scaccaglia M, Fortunato A, Alessi D, Arcudi F, Aliprandi A.   +5 more
europepmc   +1 more source

XUV fluorescence as a probe of interatomic coulombic decay of resonantly excited He nanodroplets. [PDF]

Sci Rep
Sishodia K, Ltaief LB, Scheel N, Földes IB, Roos AH, Albrecht M, Staněk M, Jurkovičová L, Hort O, Nejdl J, García-Alfonso E, Halberstadt N, Andreasson J, Klimešová E, Krikunova M, Krishnan S, Heidenreich A, Mudrich M.   +17 more
europepmc   +1 more source

Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab

Santos Ld, Owen J, Duvvuri G, Loyd ROP, Vidotto A, Presa A, Bourrier V, King G, Airapetian V, Ehrenreich D, France K, Lendl M, Lothringer J, Nielsen L.   +13 more
europepmc   +1 more source

Sensitized Photo-Oxidation of Anserine and Carnosine: Laser Flash Photolysis and CIDNP Study. [PDF]

ACS Phys Chem Au
Morozova OB, Fishman NN, Zhuravleva YS, Yurkovskaya AV.   +3 more
europepmc   +1 more source

Nucleation-Mode-Particle Emissions from Biosolid Processing Plants. [PDF]

Environ Sci Technol
Cai L, Han S, Han M, Hazelwood J, Collins A, Petters SS, Meskhidze N, Petters M.   +7 more
europepmc   +1 more source

Polarimetry of Early Emission Line Stars.

, 2001
openaire   +1 more source

Early-type emission-line stars

openaire   +1 more source

Some of the next articles are maybe not open access.

Related searches:

A survey of emission-line stars in the CMa star formation region

Astrophysics and Space Science, 1986
A survey of emission-line stars was carried out in the CMa star formation region, based on spectral observations with the Kiso Schmidt telescope. In total, 128 emission-line stars were detected, ranging from V = 6 to 15, and the majority are found with V between 11 and 14.
Suhardja D. Wiramihardja, Tomokazu Kogure, Makoto Nakano, Shigeomi Yoshida, Ken’ichi Tatematsu   +4 more
openaire   +1 more source

Emission-line Central Stars of Planetary Nebulae

AIP Conference Proceedings, 2005
The temperatures of central stars of planetary nebulae (PNe) are compared with evolutionary tracks. © 2005 American Institute of Physics.
Gesicki, K., Zijlstra, A. A.; id_orcid 0000-0002-3171-5469, Acker, A.   +2 more
openaire   +2 more sources