Results 11 to 20 of about 563,924 (339)

Organic compounds in star forming regions. [PDF]

open access: yesOrig Life Evol Biosph, 2014
The influence of complex dust composition on the general chemical evolution of a prestellar core and the content of complex organic compounds is studied. It is shown that various component groups respond differently to the presence of a small dust population.
Kochina O, Wiebe D.
europepmc   +5 more sources

Dynamical evolution of star-forming regions [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
20 pages, 9 figures, accepted for publication in ...
Richard J. Parker   +3 more
openaire   +6 more sources

Different Influence of Gas Accretion on the Evolution of Star-forming and Non-star-forming Galaxies [PDF]

open access: yesThe Astrophysical Journal
Using integral field spectroscopic data from the Mapping Nearby Galaxies at Apache Point Observatory survey, we investigate the spatially resolved properties and empirical relations of a star-forming galaxy and a non-star-forming galaxy hosting ...
Min Bao, Wenlong Zhao, Qirong Yuan
doaj   +2 more sources

Star Forming Regions in Cepheus [PDF]

open access: yesarXiv, 2008
104 pages, 25 tables, 35 figures; A chapter in the "Handbook of Star Forming Regions, Vol 1: The Northern Sky," ed. Bo Reipurth; ASP Monograph Series. Full resolution version can be found at http://www.konkoly.hu/staff/kun/handbook_chapters/
Kun, M., Kiss, Z. T., Balog, Z.
openaire   +3 more sources

Investigating the Impact of Metallicity on Star Formation in the Outer Galaxy. I. VLT/KMOS Survey of Young Stellar Objects in Canis Major

open access: yesThe Astrophysical Journal Supplement Series, 2023
The effects of metallicity on the evolution of protoplanetary disks may be studied in the outer Galaxy where the metallicity is lower than in the solar neighborhood.
Dominika Itrich   +11 more
doaj   +1 more source

Young Stellar Object Candidates in IC 417

open access: yesThe Astronomical Journal, 2023
IC 417 is in the Galactic plane, and likely part of the Aur OB2 association; it is ∼2 kpc away. Stock 8 is one of the densest cluster constituents; off of it to the east, there is a “nebulous stream” (NS) that is dramatic in the infrared (IR).
L. M. Rebull   +14 more
doaj   +1 more source

HH 80/81: Structure and Kinematics of the Fastest Protostellar Outflow

open access: yesThe Astrophysical Journal, 2023
Hubble Space Telescope (HST) images obtained in 2018 are combined with archival HST data taken in 1995 to detect changes and measure proper motions in the HH 80/81 shock complex, which is powered by the fastest known jet driven by a forming star, the ...
John Bally, Bo Reipurth
doaj   +1 more source

Membership Analysis and 3D Kinematics of the Star-forming Complex around Trumpler 37 Using Gaia-DR3

open access: yesThe Astrophysical Journal, 2023
Identifying and characterizing young populations of star-forming regions are crucial to unraveling their properties. In this regard, Gaia-DR3 data and machine-learning tools are very useful for studying large star-forming complexes.
Swagat R. Das   +4 more
doaj   +1 more source

Masers in star forming regions [PDF]

open access: yesProceedings of the International Astronomical Union, 2012
AbstractMaser emission plays an important role as a tool in star formation studies. It is widely used for deriving kinematics, as well as the physical conditions of different structures, hidden in the dense environment very close to the young stars, for example associated with the onset of jets and outflows.
Anna Bartkiewicz   +1 more
openaire   +4 more sources

Digging into the Interior of Hot Cores with ALMA: Spiral Accretion into the High-mass Protostellar Core G336.01–0.82

open access: yesThe Astrophysical Journal Letters, 2023
We observed the high-mass star-forming core G336.01–0.82 at 1.3 mm and 0.″05 (∼150 au) angular resolution with the Atacama Large Millimeter/submillimeter Array (ALMA) as part of the Digging into the Interior of Hot Cores with ALMA survey.
Fernando A. Olguin   +11 more
doaj   +1 more source

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