activity
20232026
collaborators

13 papers

astro-ph.SR2026

Hot water emission during an outburst in a classical T Tauri star

Zhen Guo, Javier Osses, Vitor Fermiano +34

In this paper, we present observations of an eruptive young star in the Rosette Nebula, identified by the Gaia Science Alerts system using Gaia time series data. We aim to investig…

astro-ph.GA2026

Investigation of Hourglass-shaped Magnetic fields in the G35.20-0.74 Star-Forming Complex

O. R. Jadhav, L. K. Dewangan, A. K. Maity +7

To investigate the role of magnetic fields toward the G35N and G35S sub-regions in the G35.20-0.74 star-forming complex, we utilized multi-wavelength polarimetric observations from…

astro-ph.GA2026

Unveiling an Hourglass-Shaped Magnetic Field toward IRDC G351.77-0.53

O. R. Jadhav, L. K. Dewangan, I. I. Zinchenko +5

We present the SOFIA/HAWC+ 214 m polarimetric observations toward the infrared dark cloud G351.77-0.53 (hereafter G351), complemented by existing multi-wavelength data sets. Inf…

astro-ph.SR2026

Gaia24ccy: An outburst followed the footsteps of its predecessor

Koshvendra Singh, Joe P. Ninan, Zhen Guo +25

Accretion-driven outbursts in young stellar objects remain poorly understood, largely limited by a statistically small sample of closely followed-up events. This underscores the im…

astro-ph.SR2025

Unveiling the Dual Nature of V1180 Cas: UXor-like Dips and EXor-like Bursts Across a Decade

Tarak Chand, Saurabh Sharma, Koshvendra Singh +15

We present a detailed analysis of the long-term photometric and spectroscopic evolution of V1180 Cas over a decade, aiming to identify the dominant mechanisms behind its variabilit…

astro-ph.SR2025

Investigating the Influence of Radiative Feedback in Bright-Rimmed Cloud 44

Rishi C, Neelam Panwar, Thomas J. Haworth +9

Radiative feedback from massive stars plays a central role in the evolution of molecular clouds and the interstellar medium. This paper presents a multi-wavelength analysis of the…

astro-ph.GA2025

Unraveling the Feedback-Regulated Star Formation Activities around the Expanding Galactic MIR Bubble [HKS2019] E71

Aayushi Verma, Saurabh Sharma, Lokesh K. Dewangan +8

We explore the physical environment of the Galactic mid-infrared (MIR) bubble [HKS2019] E71 (hereafter E71) through a multi-wavelength approach. E71 is located at the edge of a fil…

astro-ph.HE2025

Are Kronberger 80 and/or Kronberger 82 regions PeVatron candidates for LHAASO J2108+5157?

Akash Gupta, Eduardo De La Fuente, Ram K. Yadav +13

High-energy gamma rays have been detected in the region of LHAASO~J2108+5157 by the Fermi--LAT, HAWC and LHAASO-KM2A observatories. Cygnus~OB2 in Cygnus--X has been confirmed as th…

astro-ph.GA2025

Investigating Embedded Structures and Gas Kinematics in the IRDC Hosting Bubble N59-North

A. K. Maity, L. K. Dewangan, O. R. Jadhav +5

We present a multi-wavelength study of an extended area hosting the bubble N59-North to explore the physical processes driving massive star formation (MSF). The Spitzer 8 m imag…

astro-ph.GA2025

Unveiling Physical Conditions and Star Formation Processes in the G47 Filamentary Cloud

O. R. Jadhav, L. K. Dewangan, A. Haj Ismail +6

We present a multi-wavelength study of the filamentary cloud G47 (d 4.44 kpc), which hosts the mid-infrared bubbles N98, B1, and B2. The SMGPS 1.3 GHz continuum map detects i…

astro-ph.GA2024

Investigating the Star-forming Sites in the Outer Galactic Arm

Aayushi Verma, Saurabh Sharma, Lokesh K. Dewangan +7

We aim to investigate the global star formation scenario in star-forming sites AFGL 5157, [FSR2007] 0807 (hereafter FSR0807), [HKS2019] E70 (hereafter E70), [KPS2012] MWSC 0620 (he…

astro-ph.GA2024

Low-mass stellar and substellar content of the young cluster Berkeley 59

Neelam Panwar, Rishi C., Saurabh Sharma +4

We present a multi-wavelength analysis of the young star cluster Berkeley 59 (Be 59) based on the data and deep infrared (IR) observations with the 3.58-m Telescopio Naziona…

astro-ph.GA2023

Nobeyama Cygnus-X Survey: Physical Properties of CO clumps in DR-6(W), DR-9 and DR-13S regions

I. Toledano--Juárez, E. de la Fuente, K. Kawata +10

Cygnus-X is considered a region of interest for high-energy astrophysics, since the Cygnus OB2 association has been confirmed as a PeVatron in the Cygnus cocoon. In this research n…