output
19922026
most citedNeutrino Masses and Leptogenesis with Heavy Higgs Triplets

518 citations

Showing 2022 · astro-ph.GAShow all

24 papers · 2 filters

astro-ph.GA2022★ 13 cited

Search and characterization of remnant radio galaxies in the XMMLSS deep field

Sushant Dutta, Veeresh Singh, C. H. Ishwara Chandra +3

The remnant phase of a radio galaxy is characterized by the cessation of AGN activity resulting in the stoppage of jets supplying plasma to radio lobes. In this paper, we present t…

astro-ph.GA2022★ 18 cited

The mid-infrared molecular inventory towards Orion IRc2

Sarah Nickerson, Naseem Rangwala, Sean W. J. Colgan +8

We present the first high spectral resolution mid-infrared survey in the Orion BN/KL region, covering 7.2 to 28.3 micron. With SOFIA/EXES we target the enigmatic source Orion IRc2.…

astro-ph.GA2022★ 8 cited

Star-forming site RAFGL 5085: Is a perfect candidate of hub-filament system ?

L. K. Dewangan, N. K. Bhadari, A. K. Maity +4

To investigate the star formation process, we present a multi-wavelength study of a massive star-forming site RAFGL 5085, which has been associated with the molecular outflow, HII…

astro-ph.GA2022★ 9 cited

The Outer spiral arm of the Milky Way using Red Clump stars

Namita Uppal, Shashikiran Ganesh, Mathias Schultheis

Aims: Our aim is to provide an observational view of the old Disc structure of the Milky Way galaxy using the distribution of red clump stars. The spiral arms, warp structure, and…

astro-ph.GA2022★ 8 cited

Core orientations and magnetic fields in isolated molecular clouds

Ekta Sharma, Maheswar Gopinathan, Archana Soam +2

Molecular clouds are sites of star formation. Magnetic fields are believed to play an important role in their dynamics and shaping morphology. We aim to study any possible correlat…

astro-ph.GA2022★ 3 cited

Ionized filaments and ongoing physical processes in massive star-forming sites around l = 345.5 degree

L. K. Dewangan, L. E. Pirogov, N. K. Bhadari +1

Numerous research studies on dust and molecular filaments have been conducted in star-forming sites, but only a limited number of studies have focused on ionized filaments. To obse…

astro-ph.GA2022★ 3 cited

Fragmented atomic shell around S187 HII region and its interaction with molecular and ionized gas

Petr Zemlyanukha, Igor I. Zinchenko, Evgeny Dombek +6

The environment of S187, a nearby H II region (1.40.3 kpc), is analyzed. A surrounding shell has been studied in the H I line, molecular lines, and also in infrared and radio…

astro-ph.GA2022★ 14 cited

Astrochemical model to study the abundances of branched carbon-chain molecules in a hot molecular core with realistic binding energies

Satyam Srivastav, Milan Sil, Prasanta Gorai +3

Straight-chain (normal-propyl cyanide, n - C3H7CN) and branched-chain (iso-propyl cyanide, i - C3H7CN) alkyl cyanides are recently identified in the massive star-forming regions (S…

astro-ph.GA2022★ 13 cited

Tracers of Dense Gas in the Outer Galaxy

Sudeshna Patra, Neal J. Evans, Kee-Tae Kim +5

We have mapped HCN and HCO (J = 1 0) line emission toward a sample of seven star-forming regions (with 12 + log[O/H] range from 8.34 to 8.69) in the outer Milky Way (Ga…

astro-ph.GA2022★ 1 cited

Characteristics of remnant radio galaxies detected in the deep radio continuum observations from the SKA pathfinders

Sushant Dutta, Veeresh Singh, C. H. Ishwara Chandra +2

The cessation of AGN activity in radio galaxies leads to a remnant phase during which jets are no longer sustained, but lobes can be detected for a period of time before they fade…

astro-ph.GA2022★ 1 cited

Detection of radio-AGN in dust-obscured galaxies using deep uGMRT radio continuum observations

Abhijit Kayal, Veeresh Singh, C. H. Ishwara Chandra +2

Radio observations being insensitive to the dust-obscuration, have been exploited to unveil the population of Active Galactic Nuclei (AGN) residing in galaxies with large dust cont…

astro-ph.GA2022★ 86 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XI. From inflow to infall in hub-filament systems

Jian-Wen Zhou, Tie Liu, Neal J. Evans +37

We investigate the presence of hub-filament systems in a large sample of 146 active proto-clusters, using HCO J=1-0 molecular line data obtained from the ATOMS survey.…

astro-ph.GA2022★ 18 cited

Unraveling the observational signatures of cloud-cloud collision and hub-filament systems in W31

A. K. Maity, L. K. Dewangan, H. Sano +3

To understand the formation process of massive stars, we present a multi-scale and multi-wavelength study of the W31 complex hosting two extended HII regions (i.e., G10.30-0.15 (he…

astro-ph.GA2022★ 3 cited

Optical linear polarization study towards Czernik 3 open cluster at different spatial scales

Namita Uppal, Shashikiran Ganesh, D. Bisht

We present the optical linear polarization observation of stars towards the core of the Czernik 3 cluster in the Sloan i-band. The data were obtained using the EMPOL instrument on…

astro-ph.GA2022★ 13 cited

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Evidence for a Molecular Jet Launched at an Unprecedented Early Phase of Protostellar evolution

Somnath Dutta, Chin-Fei Lee, Naomi Hirano +31

Protostellar outflows and jets play a vital role in star formation as they carry away excess angular momentum from the inner disk surface, allowing the material to be transferred t…

astro-ph.GA2022★ 10 cited

New evidences in IRDC G333.73+0.37: colliding filamentary clouds, hub-filament system, and embedded cores

L. K. Dewangan

To unravel the star formation process, we present a multi-scale and multi-wavelength study of the filamentary infrared dark cloud (IRDC) G333.73+0.37, which hosts previously known…

astro-ph.GA2022★ 23 cited

Simultaneous evidence of edge collapse and hub-filament configurations: A rare case study of a Giant Molecular Filament G45.3+0.1

N. K. Bhadari, L. K. Dewangan, D. K. Ojha +2

We study multiwavelength and multiscale data to investigate the kinematics of molecular gas associated with the star-forming complexes G045.49+00.04 (G45E) and G045.14+00.14 (G45W)…

astro-ph.GA2022

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- X. Chemical differentiation among the massive cores in G9.62+0.19

Y. P. Peng, T. Liu, S. -L. Qin +23

Investigating the physical and chemical structures of massive star-forming regions is critical for understanding the formation and the early evolution of massive stars. We performe…

astro-ph.GA2022★ 20 cited

Mid-IR and VUV Spectroscopic Characterisation of Thermally Processed and Electron Irradiated CO2 Astrophysical Ice Analogues

DV Mifsud, Z Kaňuchová, S Ioppolo +19

The astrochemistry of CO2 ice analogues has been a topic of intensive investigation due to the prevalence of CO2 throughout the interstellar medium and the Solar System, as well as…

astro-ph.GA2022★ 9 cited

Understanding the impact of diffusion of CO in the astrochemical models

Kinsuk Acharyya

The mobility of lighter species on the surface of interstellar dust grains plays a crucial role in forming simple through complex molecules. Carbon monoxide is one of the most abun…

astro-ph.GA2022★ 36 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions-IX. A pilot study towards IRDC G034.43+00.24 on multi-scale structures and gas kinematics

Hong-Li Liu, Anandmayee Tej, Tie Liu +21

We present a comprehensive study of the gas kinematics associated with density structures at different spatial scales in the filamentary infrared dark cloud, G034.43+00.24 (G34). T…

astro-ph.GA2022★ 42 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- VIII. A search for hot cores by using CHCN, CHOCHO and CHOH lines

Sheng-Li Qin, Tie Liu, Xunchuan Liu +29

Hot cores characterized by rich lines of complex organic molecules are considered as ideal sites for investigating the physical and chemical environments of massive star formation.…

astro-ph.GA2022★ 10 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- VII. A catalogue of SiO clumps from ACA observations

Rong Liu, Tie Liu, Gang Chen +28

To understand the nature of SiO emission, we conducted ACA observations of the SiO (2-1) lines toward 146 massive star-forming regions, as part of the ALMA Three-millimeter Observa…

astro-ph.GA2022

Intra-night optical variability study of a non-jetted narrow-line Seyfert 1 galaxy: SDSS J163401.94+480940.1

Vineet Ojha

SDSS J163401.94480940.2 is a non-jetted radio-loud narrow-line Seyfert 1 (NLSy1) galaxy. Optical monitoring of this object was carried out in two intra-night sessions each $\geq…