Results 81 to 90 of about 200,551 (195)
Properties of the ionized gas in HH 202 – II. Results from echelle spectrophotometry with ultraviolet visual echelle spectrograph ⃰ [PDF]
We present results of deep echelle spectrophotometry of the brightest knot of the Herbig–Haro object HH 202 in the Orion Nebula – HH 202-S – using the Ultraviolet Visual Echelle Spectrograph in the spectral range from 3100 to 10 400 Å.
Monica Rodriguez
core
A Perfect Tidal Storm: HD 104067 Planetary Architecture Creating an Incandescent World
The discovery of planetary systems beyond the solar system has revealed a diversity of architectures, most of which differ significantly from our system.
Stephen R. Kane +7 more
doaj +1 more source
Novel Calibration Approach for Monitoring Aerosol Hydrogen Isotopes Using Laser-Induced Breakdown Spectroscopy for Molten Salt Reactor Off-Gas Streams. [PDF]
Andrews HB, McFarlane J.
europepmc +1 more source
Laser-induced breakdown spectroscopy (LIBS) is a method for elemental composition analysis that has been proposed for fusion reactor safety diagnostics.
Jasper Ristkok +16 more
doaj +1 more source
The California Legacy Survey. V. Chromospheric Activity Cycles in Main-sequence Stars
We present optical spectroscopy of 710 solar neighborhood stars collected over 20 years to catalog chromospheric activity and search for stellar activity cycles.
Howard Isaacson +33 more
doaj +1 more source
Field-Capable Spectrometer Module
<p>Field-Capable Spectrometer Module</p ...
Alex Gorsuch +4 more
core +1 more source
The giant planet–metallicity correlation revealed that planetary formation depends on the stellar properties. There is growing evidence that it is also valid for smaller hot planets, but it is not clear whether elements other than iron also influence the
Luan Ghezzi +3 more
doaj +1 more source
Pre-Launch Spectral Calibration of the Absorbed Aerosol Sensor. [PDF]
Mao J, Wang Y, Shi E, Wang J.
europepmc +1 more source
<p>for Poker Flat Digital Meridian Spectrometer, which uses netCDF</p ...
Michael Hirsch
core +1 more source
Measuring the distance of quasar outflows from the central source ( R ) is essential for determining their importance for active galactic nucleus feedback.
Mayank Sharma +10 more
doaj +1 more source

