Results 161 to 170 of about 29,479 (190)

Characteristics of distal femoral articular cartilage in 6 weeks posttraumatic osteoarthritis by a subcritical impact. [PDF]

open access: yesJ Orthop Res
Mantebea H   +7 more
europepmc   +1 more source

Effect of pH and temperature on the stability of the natural dye from the roselle flower (<i>Hibiscus sabdariffa</i> L.) and its application in flavored milk. [PDF]

open access: yesJ Food Sci Technol
Zuluaga-Vega J   +10 more
europepmc   +1 more source

An Overview of Appropriate Medical Practice and Preparedness in Radiation Emergency Response. [PDF]

open access: yesCureus
Al-Ibraheem A   +15 more
europepmc   +1 more source

Toxic and Hallucinogenic Plants of Southern Chile of Forensic Interest: A Review. [PDF]

open access: yesPlants (Basel)
Díaz R   +6 more
europepmc   +1 more source

Hot Rolled Strip Re-reddening Temperature Changing Law during Ultra-fast Cooling

open access: closedJournal of Iron and Steel Research International, 2015
Temperature deviation between surface and the center of hot rolled strip is formed during ultra-fast cooling (UFC). Surface temperature would rise when temperature deviation goes up to an extent, and strip re-reddening phenomenon will appear. Strip re-reddening affects the stability of strip microstructure, property and temperature control precision ...
江连运   +4 more
  +5 more sources
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On interstellar reddening law in the Taurus dark clouds

Astrophysics and Space Science, 1982
The interstellar reddening law in the Taurus dark clouds is investigated from visual, infrared, and ground based ultraviolet photometric observations of heavily reddened stars HD 29647, HDE 283701, and HDE 283812. The star HD 29647 located in the center of a very dense dark cloud Khavtassi 278 shows a reddening law which is anomalous in the wavelengths
V. Straižys   +2 more
openaire   +1 more source

UBVR colours of accretion disks and power-law sources of radiation with interstellar reddening

Astronomical & Astrophysical Transactions, 1991
Abstract The (U–B), (B–V) and (V–R) colour indexes from accretion disks, and sources with power-law spectra, are calculated. They take into account interstellar extinction, in detail. Results are given on two-colour diagrams (U–B)-(B–V) and (B–V)−(V–R). Applications to Nova Vul 1988 and A0620–00 are discussed shortly.
N. G. Bochkarev   +3 more
openaire   +1 more source

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