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View article: Magnetic Activities of GJ 1151: Flares in TESS Data and Radio Observation in uGMRT
Magnetic Activities of GJ 1151: Flares in TESS Data and Radio Observation in uGMRT Open
GJ 1151 is a nearby (8 pc), quiescent mid-M dwarf (M 4.5V) of older age, made especially interesting by the hypothesized presence of a close-in planet invoked to explain its low-frequency radio emission. We analyzed the flaring activity of…
View article: The ALMA-QUARKS Survey. III. Clump-to-core Fragmentation and Searches for High-mass Starless Cores
The ALMA-QUARKS Survey. III. Clump-to-core Fragmentation and Searches for High-mass Starless Cores Open
The Querying Underlying mechanisms of massive star formation with ALMA-Resolved gas Kinematics and Structures (QUARKS) survey observed 139 infrared-bright (IR-bright) massive protoclusters at 1.3 mm wavelength with the Atacama Large Millim…
View article: The ALMA-ATOMS Survey: Exploring Protostellar Outflows in HC$_3$N
The ALMA-ATOMS Survey: Exploring Protostellar Outflows in HC$_3$N Open
We present the first systematic study of bipolar outflows using HC$_3$N as a tracer in a sample of 146 massive star-forming regions from ALMA-ATOMS survey. Protostellar outflows arise at the initial stage of star formation as a consequence…
View article: JWST-ALMA study of a hub-filament system in the nascent phase
JWST-ALMA study of a hub-filament system in the nascent phase Open
Context. Star clusters, including high-mass stars, form within hub-filament systems (HFSs). Observations of HFSs that remain unaffected by feedback from embedded stars are rare yet crucial for understanding the mass inflow process in high-…
View article: JWST-ALMA Study of a Hub-Filament System in the Nascent Phase
JWST-ALMA Study of a Hub-Filament System in the Nascent Phase Open
Star clusters, including high-mass stars, form within hub-filament systems (HFSs). Observations of HFSs that remain unaffected by feedback from embedded stars are rare yet crucial for understanding the mass inflow process in high-mass star…
View article: The Milky Way atlas for linear filaments – II. Clump rotation versus filament orientation
The Milky Way atlas for linear filaments – II. Clump rotation versus filament orientation Open
Dense clumps distributed along filaments are the immediate medium for star formation. Kinematic properties of the clumps, such as velocity gradient and angular momentum, combined with filament orientation, provide important clues to the fo…
View article: The Milky Way atlas for linear filaments II. clump rotation versus filament orientation
The Milky Way atlas for linear filaments II. clump rotation versus filament orientation Open
Dense clumps distributed along filaments are the immediate medium for star formation. Kinematic properties of the clumps, such as velocity gradient and angular momentum, combined with filament orientation, provide important clues to the fo…
View article: Detection of High-frequency Pulsation in WR 135: Investigation of Stellar Wind Dynamics
Detection of High-frequency Pulsation in WR 135: Investigation of Stellar Wind Dynamics Open
We report the detection of high-frequency pulsations in WR 135 from short-cadence (10 minute) optical photometric and spectroscopic time series surveys. The harmonics up to the sixth order are detected from the integrated photometric flux …
View article: ALMA-IMF. XIV. Free–Free Templates Derived from H41α and Ionized Gas Content in 15 Massive Protoclusters
ALMA-IMF. XIV. Free–Free Templates Derived from H41α and Ionized Gas Content in 15 Massive Protoclusters Open
We use the H41 α recombination line to create templates of the millimeter free–free emission in the ALMA-IMF continuum maps, which allows us to separate it from dust emission. This method complements spectral-index information and extrapol…
View article: Direct Observational Evidence of Multi-epoch Massive Star Formation in G24.47+0.49
Direct Observational Evidence of Multi-epoch Massive Star Formation in G24.47+0.49 Open
Using new continuum and molecular line data from the Atacama Large Millimeter/submillimeter Array Three-millimeter Observations of Massive Star-forming Regions (ATOMS) survey and archival Very Large Array, 4.86 GHz data, we present direct …
View article: ALMA-IMF XV: The core mass function in the high-mass star-formation regime
ALMA-IMF XV: The core mass function in the high-mass star-formation regime Open
The stellar initial mass function (IMF) is critical to our understanding of star formation and the effects of young stars on their environment. On large scales, it enables us to use tracers such as UV or Halpha emission to estimate the sta…
View article: ALMA-IMF XIV: Free-Free Templates Derived from H$41α$ and Ionized Gas Content in Fifteen Massive Protoclusters
ALMA-IMF XIV: Free-Free Templates Derived from H$41α$ and Ionized Gas Content in Fifteen Massive Protoclusters Open
We use the H$41α$ recombination line to create templates of the millimeter free-free emission in the ALMA-IMF continuum maps, which allows to separate it from dust emission. This method complements spectral-index information and extrapolat…
View article: Direct observational evidence of multi-epoch massive star formation in G24.47+0.49
Direct observational evidence of multi-epoch massive star formation in G24.47+0.49 Open
Using new continuum and molecular line data from the ALMA Three-millimeter Observations of Massive Star-forming Regions (ATOMS) survey and archival VLA, 4.86 GHz data, we present direct observational evidence of hierarchical triggering rel…
View article: ALMA-IMF
ALMA-IMF Open
The ALMA-IMF Large Program provides multi-tracer observations of 15 Galactic massive protoclusters at a matched sensitivity and spatial resolution. We focus on the dense gas kinematics of the G353.41 protocluster traced by N 2 H + (1−0), w…
View article: Investigation of [KSF2015] 1381-19L, a WC9-type Star in the High-extinction Galactic Region
Investigation of [KSF2015] 1381-19L, a WC9-type Star in the High-extinction Galactic Region Open
We report on a multiwavelength study of the Wolf–Rayet star [KSF2015] 1381-19L, which is located in the solar metallicity region ( Z = 0.014) of the Milky Way, strongly obscured by interstellar dust. We perform a detailed characterization …
View article: Influence of mid-infrared Galactic bubble on surroundings: A case study on IRAS 16489-4431
Influence of mid-infrared Galactic bubble on surroundings: A case study on IRAS 16489-4431 Open
We studied the influence of a massive star on a mid-infrared bubble and its surrounding gas in the IRAS\,16489-4431 star-forming region using multi-wavelength data. The {\it Spitzer} mid-infrared band images revealed the shocked nature of …
View article: The Milky Way atlas for linear filaments
The Milky Way atlas for linear filaments Open
Context. Filamentary structure is important for the ISM and star formation. Galactic distribution of filaments may regulate the star formation rate in the Milky Way. However, interstellar filaments are intrinsically complex, making them di…
View article: Detection of high-frequency pulsation in WR 135: investigation of stellar wind dynamics
Detection of high-frequency pulsation in WR 135: investigation of stellar wind dynamics Open
We report the detection of high-frequency pulsations in WR\,135 from short cadence (10\,minutes) optical photometric and spectroscopic time series surveys. The harmonics up to $6^{th}$ order are detected from the integrated photometric flu…
View article: Study of Complex Nitrogen and Oxygen-bearing Molecules toward the High-mass Protostar IRAS 18089–1732
Study of Complex Nitrogen and Oxygen-bearing Molecules toward the High-mass Protostar IRAS 18089–1732 Open
The observation of oxygen (O)- and nitrogen (N)-bearing molecules gives an idea about the complex prebiotic chemistry in the interstellar medium. Recent millimeter and submillimeter wavelength observations have shown the presence of comple…
View article: Star Formation in the H ii Region Sh2-87: Evidence of Global Hierarchical Collapse
Star Formation in the H ii Region Sh2-87: Evidence of Global Hierarchical Collapse Open
We present a detailed study of the Sh2-87 H ii region using a multiwavelength data set in optical to radio bands. A Herschel column density map revealed that the host cloud is filamentary in nature, and together they formed a central dense…
View article: The ALMA-QUARKS Survey: Detection of Two Extremely Dense Substructures in a Massive Prestellar Core
The ALMA-QUARKS Survey: Detection of Two Extremely Dense Substructures in a Massive Prestellar Core Open
Only a handful of massive starless core candidates have been discovered so far, but none of them have been fully confirmed. Within the MM1 clump in the filamentary infrared dark cloud G34.43+0.24 that was covered by the Atacama Large Milli…
View article: Deciphering the hidden structures of HH 216 and Pillar IV in M16: results from <i>JWST</i> and <i>HST</i>
Deciphering the hidden structures of HH 216 and Pillar IV in M16: results from <i>JWST</i> and <i>HST</i> Open
To probe the star formation process, we present an observational investigation of the Pillar IV and an ionized knot HH 216 in the Eagle Nebula (M16). Pillar IV is known to host a Class I protostar that drives a bipolar outflow. The outflow…
View article: Deciphering the Hidden Structures of HH 216 and Pillar IV in M16: Results from JWST and HST
Deciphering the Hidden Structures of HH 216 and Pillar IV in M16: Results from JWST and HST Open
To probe the star formation process, we present an observational investigation of the Pillar IV and an ionized knot HH 216 in the Eagle Nebula (M16). Pillar IV is known to host a Class I protostar that drives a bipolar outflow. The outflow…
View article: The ALMA-QUARKS survey: Detection of two extremely dense substructures in a massive prestellar core
The ALMA-QUARKS survey: Detection of two extremely dense substructures in a massive prestellar core Open
Only a handful of massive starless core candidates have been discovered so far, but none of them have been fully confirmed. Within the MM1 clump in the filamentary infrared dark cloud G34.43+0.24 that was covered by the ALMA-ATOMS survey a…
View article: Proceedings of the 3rd BINA Workshop: Scientific Potential of Indo-Belgian Co-operation
Proceedings of the 3rd BINA Workshop: Scientific Potential of Indo-Belgian Co-operation Open
In this report, we present an overview of the 3rd BINA workshop hosted by ARIES, Nainital on a broad theme the Scientific potential of the Indo-Belgian co-operation. Further, an introduction of the proceedings of the 3rd BINA workshop is a…
View article: ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters Open
We present a catalog of 315 protostellar outflow candidates detected in SiO J = 5 − 4 in the ALMA-IMF Large Program, observed with ∼2000 au spatial resolution, 0.339 km s −1 velocity resolution, and 2–12 mJy beam −1 (0.18–0.8 K) sensitivit…
View article: Feedback from protoclusters does not significantly change the kinematic properties of the embedded dense gas structures
Feedback from protoclusters does not significantly change the kinematic properties of the embedded dense gas structures Open
A total of 64 ATOMS sources at different evolutionary stages were selected to investigate the kinematics and dynamics of gas structures under feedback. We identified dense gas structures based on the integrated intensity map of H 13 CO + J…
View article: Feedback from protoclusters does not significantly change the kinematic properties of the embedded dense gas structures
Feedback from protoclusters does not significantly change the kinematic properties of the embedded dense gas structures Open
A total of 64 ATOMS sources at different evolutionary stages were selected to investigate the kinematics and dynamics of gas structures under feedback. We identified dense gas structures based on the integrated intensity map of H$^{13}$CO$…
View article: Observational Evidence of the Merging of Filaments and Hub Formation in G083.097+03.270
Observational Evidence of the Merging of Filaments and Hub Formation in G083.097+03.270 Open
We uncover a hub–filament system correlated with massive young stellar associations in G083.097+03.270. Diagnosed with simultaneous 12 CO, 13 CO, and C 18 O line observations, the region is found to host two distinct and elongated filament…
View article: Figure Sets, Catalog Tables, and Other Technical Materials Related to "ALMA-IMF IX: Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters"
Figure Sets, Catalog Tables, and Other Technical Materials Related to "ALMA-IMF IX: Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters" Open
This Zenodo DOI contains additional data products and technical files for the publication "ALMA-IMF IX: Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters" (Towner et al. 2024). All files, metadata, a…