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A Cloud-Scale View of the Molecular Gas Disk in the Whirlpool Galaxy and Beyond [PDF]

open access: diamondEPJ Web of Conferences, 2022
The nearby galaxy M51 (also known as the Whirlpool galaxy) hosts an iconic grand-design spiral pattern and both IRAM facilities conducted the first cloud-scale (∼50 pc resolution) survey of the molecular gas reservoir across a the disk of a massive star ...
Schinnerer Eva   +8 more
doaj   +2 more sources

Waves on the surface of the Orion molecular cloud [PDF]

open access: green, 2010
Massive stars influence their parental molecular cloud, and it has long been suspected that the development of hydrodynamical instabilities can compress or fragment the cloud. Identifying such instabilities has proved difficult.
A Rodriguez-Franco   +28 more
core   +5 more sources

Molecular Cloud Evolution VI. Measuring cloud ages [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
This article has been published in Monthly Notices of the Royal Astronomical Society © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
Ansdell   +84 more
core   +4 more sources

The Molecular Cloud Lifecycle. [PDF]

open access: yesSpace Sci Rev, 2020
AbstractGiant molecular clouds (GMCs) and their stellar offspring are the building blocks of galaxies. The physical characteristics of GMCs and their evolution are tightly connected to galaxy evolution. The macroscopic properties of the interstellar medium propagate into the properties of GMCs condensing out of it, with correlations between e.g.
Chevance M   +8 more
europepmc   +5 more sources

Ice-nucleating particles in northern Greenland: annual cycles, biological contribution and parameterizations [PDF]

open access: yesAtmospheric Chemistry and Physics, 2023
Ice-nucleating particles (INPs) can initiate ice formation in clouds at temperatures above −38 ∘C through heterogeneous ice nucleation. As a result, INPs affect cloud microphysical and radiative properties, cloud lifetime, and precipitation behavior and
K. C. H. Sze   +7 more
doaj   +1 more source

Nebula-Relay Hypothesis: The Chirality of Biological Molecules in Molecular Clouds

open access: yesFrontiers in Astronomy and Space Sciences, 2022
The chiral puzzle of biological molecules is thought to be closely related to the origin of life and is still a mystery so far. Previously, we proposed a new model on the origin of life, Nebula-Relay hypothesis, which assumed that the life on Earth ...
Lei Feng, Lei Feng, Lei Feng
doaj   +1 more source

12 CO, 13CO, AND C18 OBSERVATIONS TOWARD OMC-1 [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2002
Interstellar cabon monoxide and its isotopes were observed with the 13.7m radio telescope of the Daeduk Radio Astronomy Observatory toward Orion Molecular Cloud-1 (OMC-1).
Mun-Suk Chun   +2 more
doaj   +1 more source

Anatomy of Orion Molecular Clouds—The Astrochemistry Perspective/Approach

open access: yesFrontiers in Astronomy and Space Sciences, 2021
The Orion molecular cloud (OMC) complex is the nearest and perhaps the best-studied giant molecular cloud complex within which low-mass and massive star formation occur. A variety of molecular species, from diatomic molecules to complex organic molecules
Dipen Sahu, Sheng-Yuan Liu, Tie Liu
doaj   +1 more source

A Velocity Structure Analysis of Giant Molecular Cloud Associated with HII Region S152 [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2005
S152 is a small bright emission nebula located in the Perseus arm. Its optical diameter corresponds to 1.5 pc for an adopted distance 3.5 kpc. However, S152 is a part of a giant molecular cloud complex, which consists of several dense cores, containing ...
Woo-Yeol Choi   +3 more
doaj   +1 more source

THE CALIFORNIA MOLECULAR CLOUD [PDF]

open access: yesThe Astrophysical Journal, 2009
Accepted for publication in the ApJ. This submission has low resolution figures. Preprint with full resolution figures can be found at http://www.cfa.harvard.edu/~clada/pubs_html/California ...
C. J. Lada, M. Lombardi, J. F. Alves
openaire   +2 more sources

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