Results 41 to 50 of about 101,515 (208)
The evolution of galaxies depends on their masses and local environments; understanding when and how environmental quenching starts to operate remains a challenge.
A. Trudeau +10 more
doaj +1 more source
The spectral line energy distribution of carbon monoxide contains information about the physical conditions of the star-forming molecular hydrogen gas; however, the relation to local radiation field properties is poorly constrained.
Laura Lenkić +8 more
doaj +1 more source
GREAT: the SOFIA high-frequency heterodyne instrument
We describe the design and construction of GREAT, the German REceiver for Astronomy at Terahertz frequencies operated on the Stratospheric Observatory for Infrared Astronomy (SOFIA).
Becklin +17 more
core +1 more source
Balloon-borne three-meter telescope for far-infrared and submillimeter astronomy [PDF]
The scientific objectives, engineering analysis and design, results of technology development, and focal-plane instrumentation for a two-meter balloon-borne telescope for far-infrared and submillimeter astronomy are presented.
Fazio, Giovanni G. +2 more
core +7 more sources
We propose a new amorphous dust emission model based on the soft-potential (SP) model, applicable in the long-wavelength range from the far-infrared to the microwave.
Masashi Nashimoto
doaj +1 more source
Polarimetry in the Visible and Infrared: Application to CMB Polarimetry
Interstellar polarization from aligned dust grains can be measured both in transmission at visible and near-infrared wavelengths and in emission at far-infrared and sub-mm wavelengths.
Fosalba +6 more
core +1 more source
Focal Plane Optics In Far-Infrared And Submillimeter Astronomy [PDF]
The construction of airborne observatories, high mountaintop observatories, and space observatories designed especially for infrared and submillimeter astronomy has opened fields of research requiring new optical techniques. A typical far-IR photometric study involves measurement of a continuous spectrum in several passbands between ~30 µm and 1000 µm ...
openaire +1 more source
Mid- to Far-Infrared spectroscopy of Sharpless 171 [PDF]
We have collected one-dimensional raster-scan observations of the active star-forming region Sharpless 171 (S171), a typical HII region-molecular cloud complex, with the three spectrometers (LWS, SWS, and PHT-S) on board ISO.
Baluteau +55 more
core +1 more source
Far-infrared Luminosity Bursts Trace Mass Accretion onto Protostars
Evidence abounds that young stellar objects undergo luminous bursts of intense accretion that are short compared to the time it takes to form a star. It remains unclear how much these events contribute to the main-sequence masses of the stars.
William J. Fischer +8 more
doaj +1 more source
The ISOPHOT-MAMBO survey of 3CR radio sources: Further evidence for the unified schemes
We present the complete set of ISOPHOT observations of 3CR radio galaxies and quasars, which are contained in the ISO Data Archive, providing 75 mid- and far-infrared spectral energy distributions (SEDs) between 5 and 200 micron.
Akujor +81 more
core +1 more source

