Results 91 to 100 of about 1,217 (186)
Carbon plays key roles in the interstellar medium (ISM)—as a constituent of dust, as the carrier of the dominant far-infrared (FIR) cooling line, and as a component of various important molecules.
Christopher J. R. Clark +7 more
doaj +1 more source
We present new high-resolution ( R ∼ 114,000), near-ultraviolet spectra in the direction of 36 nearby (
Azmain H. Nisak +4 more
doaj +1 more source
We present an extragalactic H i 21 cm absorption lines catalog from a blind search at z ≤ 0.35, using drift-scan data collected in 1325.6 hr by the ongoing Commensal Radio Astronomy Fast Survey and FAST All Sky H i Survey, which spans a sky area of 6072 ...
Wenkai Hu +15 more
doaj +1 more source
Interstellar absorption lines in the directions of extragalactic objects – I [PDF]
J. C. Blades, Donald C. Morton
openaire +1 more source
Polarization of interstellar molecular radiofrequency absorption lines
N. D. Kylafis, P. R. Shapiro
openaire +1 more source
Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
europepmc +1 more source
Wavelength-dependent photofragmentation of pyrazine. [PDF]
Payra SS, Thakkar P, Lenka Y, Aravind G.
europepmc +1 more source
Rotationally Resolved Predissociation Spectrum of the 1<sup>5</sup>Φ ← X<sup>5</sup>Δ Rovibronic Band of FeH. [PDF]
Jin S +4 more
europepmc +1 more source
Laboratory detection and rotational spectroscopy of <i>trans</i>-HNSO: implications for astronomical observations. [PDF]
Lattanzi V +4 more
europepmc +1 more source

