Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
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 …
M31 satellite masses compared to ΛCDM subhaloes
EJ Tollerud, M Boylan-Kolchin… - Monthly Notices of the …, 2014 - academic.oup.com
We compare the kinematics of M31's satellite galaxies to the mass profiles of the subhaloes
they are expected to inhabit in the Λ cold dark matter (ΛCDM) cosmology. We consider the …
they are expected to inhabit in the Λ cold dark matter (ΛCDM) cosmology. We consider the …
Infrared observations of the flaring maser source G358. 93− 0.03-SOFIA confirms an accretion burst from a massive young stellar object
B Stecklum, V Wolf, H Linz, AC o Garatti… - Astronomy & …, 2021 - aanda.org
Context. Class II methanol masers are signposts of massive young stellar objects (MYSOs).
Recent evidence shows that flares of these masers are driven by MYSO accretion bursts …
Recent evidence shows that flares of these masers are driven by MYSO accretion bursts …
The accretion burst of the massive young stellar object G323. 46− 0.08
V Wolf, B Stecklum, AC o Garatti, PA Boley… - Astronomy & …, 2024 - aanda.org
Context. Accretion bursts from low-mass young stellar objects (YSOs) have been known for
many decades. In recent years, the first accretion bursts of massive YSOs (MYSOs) have …
many decades. In recent years, the first accretion bursts of massive YSOs (MYSOs) have …
The 6-GHz methanol multibeam maser catalogue–V. Galactic longitudes 20°–60°
SL Breen, GA Fuller, JL Caswell… - Monthly Notices of …, 2015 - academic.oup.com
We present the fifth portion of an unbiased survey of the Galactic plane,| b|≤ 2°, for 6668-
MHz methanol masers. This section of the survey completes the Galactic longitude range …
MHz methanol masers. This section of the survey completes the Galactic longitude range …
The Bolocam Galactic Plane Survey. XIV. Physical Properties of Massive Starless and Star-forming Clumps
BE Svoboda, YL Shirley, C Battersby… - The Astrophysical …, 2016 - iopscience.iop.org
We sort 4683 molecular clouds between 10< ℓ< 65 from the Bolocam Galactic Plane Survey
based on observational diagnostics of star formation activity: compact 70 μm sources, mid-IR …
based on observational diagnostics of star formation activity: compact 70 μm sources, mid-IR …
[HTML][HTML] The earliest phases of high-mass star formation, as seen in NGC 6334 by Herschel-HOBYS
J Tigé, F Motte, D Russeil, A Zavagno… - Astronomy & …, 2017 - aanda.org
Aims. To constrain models of high-mass star formation, the Herschel-HOBYS key program
aims at discovering massive dense cores (MDCs) able to host the high-mass analogs of low …
aims at discovering massive dense cores (MDCs) able to host the high-mass analogs of low …
Southern class I methanol masers at 36 and 44 GHz
MA Voronkov, JL Caswell, SP Ellingsen… - Monthly Notices of …, 2014 - academic.oup.com
Abstract The Australia Telescope Compact Array (ATCA) has been used for high angular
resolution imaging of 71 southern class I methanol maser sources quasi-simultaneously at …
resolution imaging of 71 southern class I methanol maser sources quasi-simultaneously at …
Methanol masers in NGC 253 with ALCHEMI
PK Humire, C Henkel, A Hernández-Gómez… - Astronomy & …, 2022 - aanda.org
Context. Methanol masers of Class I (collisionally pumped) and Class II (radiatively pumped)
have been studied in great detail in our Galaxy in a variety of astrophysical environments …
have been studied in great detail in our Galaxy in a variety of astrophysical environments …
Observations of high-order multiplicity in a high-mass stellar protocluster
The dominant mechanism forming multiple stellar systems in the high-mass regime (M*≳ 8
M⊙) remained unknown because direct imaging of multiple protostellar systems at early …
M⊙) remained unknown because direct imaging of multiple protostellar systems at early …