Search Publications

Search and study of young infrared stellar clusters
DOI: 10.1007/s10509-024-04298-3 Bibcode: 2024Ap&SS.369...33A

Azatyan, Naira

The main aim of this paper is to study both the Interstellar Medium (ISM) and the young stellar population in the three star-forming regions, namely IRAS 05137+3919, 05168+3634, and 19110+1045. The study of the ISM includes determination of the hydrogen column density (N(H2)) and dust temperature (Td) in the regions using mod…

2024 Astrophysics and Space Science
Herschel 0
The structure of the IRAS05168+3634 star-forming region
DOI: 10.1007/s10509-021-04023-4 Bibcode: 2021Ap&SS.366..114N

Nikoghosyan, E. H.; Azatyan, N. M.; Andreasyan, D. H. +1 more

This study aims to determine the main physical parameters (N(H2) hydrogen column density and Td dust temperature) of the Interstellar medium, and their distribution in the extended star-forming region, which includes IRAS 05156+3643, 05162+3639, 05168+3634, 05177+3636, and 05184+3635 sources. We also provide a comparative ana…

2021 Astrophysics and Space Science
Gaia Herschel 1
Protostellar classification using supervised machine learning algorithms
DOI: 10.1007/s10509-018-3418-7 Bibcode: 2018Ap&SS.363..197M

Miettinen, O.

Classification of young stellar objects (YSOs) into different evolutionary stages helps us to understand the formation process of new stars and planetary systems. Such classification has traditionally been based on spectral energy distribution (SED) analysis. An alternative approach is provided by supervised machine learning algorithms, which can …

2018 Astrophysics and Space Science
Herschel 12
Study of magnetic field geometry and extinction in Bok globule CB130
DOI: 10.1007/s10509-016-2905-y Bibcode: 2016Ap&SS.361..321C

Das, H. S.; Chakraborty, A.

We trace the peripheral magnetic field structure of Bok globule CB130 by estimating the linear polarization of its field stars in the R band. The magnetic field orientation sampled by these stars, aligned on average among themselves, and the polarization produced within the cloud has a different direction from that of Galactic plane with an offset…

2016 Astrophysics and Space Science
Herschel 12
KOSMA 12CO(2–1) and (3–2) observations toward Infrared Dark Clouds
DOI: 10.1007/s10509-016-2807-z Bibcode: 2016Ap&SS.361..220L

Li, Dalei; Tang, Xindi; Zhou, Jianjun +7 more

Infrared Dark Clouds (IRDCs) are a valuable sample to study the initial conditions and the very early stages of the evolution of massive stars. Using the KOSMA telescope, we performed simultaneous single point 12CO(2–1) and (3–2) observations toward 117 IRDCs with a detection rate of 74 % for 12CO(2–1) and 58 % for 12

2016 Astrophysics and Space Science
Herschel 1
The far-infrared properties of broad absorption line quasars from the Sloan Digital Sky Survey
DOI: 10.1007/s10509-015-2322-7 Bibcode: 2015Ap&SS.357....3P

Pu, Xingting

We present the results of a study which uses a sample of 320 Sloan Digital Sky Survey (SDSS) quasars with 1.68≤z≤2.28 inside the Herschel Stripe 82 Survey (HerS) region to compare the mid-infrared (MIR) and far-infrared (FIR) properties of broad absorption line (BAL) and non-BAL quasars. The BAL quasar sample comprises 56 high-ionization BAL (HiBA…

2015 Astrophysics and Space Science
Herschel 2
Global spectral energy distributions of the Large Magellanic Cloud with interstellar dust
DOI: 10.1007/s10509-013-1641-9 Bibcode: 2014Ap&SS.349..423K

Chung, Eun Jung; Kim, Sungeun; Kwon, Eunjoo +3 more

The effects of dust on infrared emission vary among galaxies of different morphological types. We investigated integrated spectral energy distributions (SEDs) in infrared and submillimeter/millimeter emissions from the Large Magellanic Cloud (LMC) based on observations from the Herschel Space Observatory (HSO) and near- to mid-infrared observation…

2014 Astrophysics and Space Science
Herschel 1