Results 61 to 70 of about 705,440 (315)
Hydrogen Fluoride in High-Mass Star-forming Regions [PDF]
Hydrogen fluoride has been established to be an excellent tracer of molecular hydrogen in diffuse clouds. In denser environments, however, the HF abundance has been shown to be approximately two orders of magnitude lower.
Ceccarelli, Cecilia +7 more
core +4 more sources
Galaxy Interactions in Compact Groups II: abundance and kinematic anomalies in HCG 91c [PDF]
Galaxies in Hickson Compact Group 91 (HCG 91) were observed with the WiFeS integral field spectrograph as part of our ongoing campaign targeting the ionized gas physics and kinematics inside star forming members of compact groups.
Borthakur, S. +6 more
core +2 more sources
UVIT Imaging of WLM: Demographics of Star-forming Regions in the Nearby Dwarf Irregular Galaxy [PDF]
We present a study of star-forming regions and their demographics in the nearby dwarf irregular galaxy WLM using Ultraviolet Imaging Telescope (UVIT) multiband observations in three filters, F148W, N245M, and N263M.
C. Mondal, A. Subramaniam, K. George
semanticscholar +1 more source
Star-forming Clumps in Local Luminous Infrared Galaxies [PDF]
We present HST narrowband near-infrared imaging of Paα and Paβ emission of 48 local luminous infrared galaxies (LIRGs) from the Great Observatories All-Sky LIRG Survey.
Armus, L. +17 more
core +3 more sources
Seeds Of Life In Space (SOLIS): The Organic Composition Diversity at 300–1000 au Scale in Solar-type Star-forming Regions [PDF]
Complex organic molecules have been observed for decades in the interstellar medium. Some of them might be considered as small bricks of the macromolecules at the base of terrestrial life.
C. Ceccarelli +56 more
semanticscholar +1 more source
Star-Forming Regions in the SMC [PDF]
AbstractSMC has been going through an active star formation epoch, especially during the last 0.2 Gyr when the close encounter with the LMC occured. Our goal is to detect regions dominated by early-type stars and gas and examine their behaviour at different wavelengths.
E. Kontizas +8 more
openaire +2 more sources
Formation of ethylene glycol and other complex organic molecules in star-forming regions [PDF]
Context. The detection of complex organic molecules related with prebiotic chemistry in star-forming regions allows us to investigate how the basic building blocks of life are formed. Aims.
V. Rivilla +5 more
semanticscholar +1 more source
Ices in star forming regions [PDF]
IR spectra of sources associated with molecular cloud material show a variety of absorption features attributed to simple molecules, such as H2O, CO, CH3OH, CO2, CH4, and OCS in icy grain mantles. These identifications are reviewed. These molecules are formed through accretion and reaction of gas phase species on grain surfaces.
Alexander G. G. M. Tielens +1 more
openaire +2 more sources
The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region [PDF]
Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower metallicity than the Sun and older clusters in the solar vicinity.
Adibekyan, V. +39 more
core +2 more sources
The field of astrochemistry concerns the formation and abundance of molecules in the interstellar medium, star-forming regions, exoplanets, and solar system bodies.
I. Cooke, I. Sims
semanticscholar +1 more source

