ATLASGAL–evolutionary trends in high-mass star formation
ABSTRACT ATLASGAL is an 870-µm dust survey of 420 deg2 the inner Galactic plane and
has been used to identify∼ 10 000 dense molecular clumps. Dedicated follow-up …
has been used to identify∼ 10 000 dense molecular clumps. Dedicated follow-up …
OMC-2 FIR 4 under the microscope: Shocks, filaments, and a highly collimated jet at 100 au scales
L Chahine, A López-Sepulcre, L Podio… - Astronomy & …, 2022 - aanda.org
Context. Star-forming molecular clouds are characterised by the ubiquity of intertwined
filaments. The filaments have been observed in both high-and low-mass star-forming …
filaments. The filaments have been observed in both high-and low-mass star-forming …
ATLASGAL: 3 mm class I methanol masers in high-mass star formation regions
Context. Class I methanol masers are known to be associated with shocked outflow regions
around massive protostars, indicating a possible link between the maser properties and …
around massive protostars, indicating a possible link between the maser properties and …
Hyperfine structure of the methanol molecule as traced by Class I methanol masers
II Agafonova, OS Bayandina, Y Gong… - Monthly Notices of …, 2024 - academic.oup.com
We present results on simultaneous observations of Class I methanol masers at 25, 36, and
44 GHz towards 22 Galactic targets carried out with the Effelsberg 100-m telescope. The …
44 GHz towards 22 Galactic targets carried out with the Effelsberg 100-m telescope. The …
Water masers as an early tracer of star formation
DA Ladeyschikov, Y Gong, AM Sobolev… - The Astrophysical …, 2022 - iopscience.iop.org
We present a study of the correlation between 22 GHz water maser emission and far-
infrared/submillimeter (IR/sub-mm) sources. The generalized linear model (GLM) is used to …
infrared/submillimeter (IR/sub-mm) sources. The generalized linear model (GLM) is used to …
Probing infrared dark clouds with class I methanol masers and thermal molecular emission using the Onsala 20 meter telescope
NN Shakhvorostova, AV Alakoz… - Monthly Notices of …, 2023 - academic.oup.com
Infrared dark clouds (IRDCs) represent the earliest stage of high-mass star formation and
host molecular cores at different states of activity from quiet state without any IR-signature of …
host molecular cores at different states of activity from quiet state without any IR-signature of …
Online Database of Multiwavelength Water Masers in Galactic Star-forming Regions
DA Ladeyschikov, AM Sobolev… - The Astronomical …, 2022 - iopscience.iop.org
In this paper, we present an online multiwavelength database of water masers in star-
forming regions of the Galaxy. The collected data represent∼ 95% of all observations of …
forming regions of the Galaxy. The collected data represent∼ 95% of all observations of …
Evolutionary Trends in Star Formation
JS Urquhart - Proceedings of the International Astronomical Union, 2022 - cambridge.org
Over the past 20 years, the Galactic plane has been surveyed at high resolution at
wavelengths from 1 micron through to 20 cm. The combination of these surveys has …
wavelengths from 1 micron through to 20 cm. The combination of these surveys has …
HIGH MASS STAR FORMATION AND METHANOL MASERS
N Wilson - 2022 - via.library.depaul.edu
Abstract Class I and Class II methanol (CH3OH) masers are believed to be good indicators
for regions where high mass stars are being formed. High mass stars are important because …
for regions where high mass stars are being formed. High mass stars are important because …
Онлайн-база данных водяных мазеров в областях звездообразования: первые результаты
ДА Ладейщиков - Астрономия и исследование космического …, 2021 - elar.urfu.ru
Представлены первые результаты разработки базы данных водяных мазеров в
областях звездообразования. База данных в настоящий момент доступна в режиме …
областях звездообразования. База данных в настоящий момент доступна в режиме …