activity
20162026
most citedA Systematic Study of the dust of Galactic Supernova Remnants I. The Distance and the Extinction

49 citations · 308 across the 20 of their papers we have counts for

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Showing astro-ph.GAShow all

12 papers · 1 filter

astro-ph.GA2026

Estimation of Dust Mass from Infrared Emission and Extinction of Supernova Remnants: G93.7-0.2, G109.1-1.0, G156.2+5.7, and G166.0+4.3

Zhe Zhang, Jun Li, Biwei Jiang +1

Supernova remnants (SNRs) are major sites for both the production and destruction of interstellar dust, and quantifying their dust budget is essential for understanding the life cy…

astro-ph.GA2026

Distance Determination of Southern Galactic Plane Supernova Remnants with the Mopra CO Survey and DECaPS 3D Dust Map

Fupeng Liu, He Zhao, Biwei Jiang +2

Accurate distance measurements to supernova remnants (SNRs) are crucial for understanding their physical properties, evolutionary processes, and role in the Galactic interstellar m…

astro-ph.GA2026

Radiative Compression of Dense Cores in the Pillars of Creation as Revealed by JWST Extinction Mapping

Jun Li, Bingqiu Chen, He Zhao +2

The Pillars of Creation in M16 represent an iconic star-forming region where stellar feedback shapes molecular cloud evolution. We present a detailed investigation of dust extincti…

astro-ph.GA2024

Spatial Variations of Dust Opacity and Grain Growth in Dark Clouds: L1689, L1709 and L1712

Jun Li, Biwei Jiang, He Zhao +2

The far-infrared (FIR) opacity of dust in dark clouds within the Ophiuchus molecular cloud is investigated through multi-wavelength infrared observations from UKIDSS, Spitzer and H…

astro-ph.GA2022★ 15 cited

Peering into the Milky Way by FAST: IV. Identification of two new Galactic supernova remnants G203.1+6.6 and G206.7+5.9

X. Y. Gao, W. Reich, X. H. Sun +5

A 5 7 sky area containing two large radio structures of G203.1+6.6 and G206.7+5.9 with a size of about 2.5 and 3.5 respectively is…

astro-ph.GA2022★ 3 cited

The Pristine Inner Galaxy Survey (PIGS) VI: Different vertical distributions between two DIBs at 442.8 nm and 862.1 nm

He Zhao, Mathias Schultheis, Anke Arentsen +8

Although diffuse interstellar bands (DIBs) were discovered over 100 years ago, for most of them, their origins are still unknown. Investigation on the correlations between differen…

astro-ph.GA2021★ 3 cited

The Dust Mass of Supernova Remnants in M31

Ye Wang, Biwei Jiang, Jun Li +2

The dust temperature and mass of the supernova remnants (SNRs) in M31 are estimated by fitting the infrared spectral energy distribution calculated from the images in the Spitzer/I…

astro-ph.GA2021★ 19 cited

The Extinction and Distance of the MBM Molecular Clouds at High Galactic Latitude

Mingxu Sun, Biwei Jiang, He Zhao +1

Based on the accurate color excess of more than 4 million stars and of more than 1 million stars from \citet{2021ApJS..254...38S}, the…

astro-ph.GA2020★ 9 cited

The distances to molecular clouds in the fourth Galactic quadrant

Chen Bingqiu, Wang Shu, Hou Ligang +4

Distance measurements to molecular clouds are essential and important. We present directly measured distances to 169 molecular clouds in the fourth quadrant of the Milky Way. Based…

astro-ph.GA2020★ 36 cited

Distances to the Supernova Remnants in the Inner Disk

Shu Wang, Chengyu Zhang, Biwei Jiang +5

Distance measurements of supernova remnants (SNRs) are essential and important. Accurate estimates of physical size, dust masses, and some other properties of SNRs depend criticall…

astro-ph.GA2018★ 36 cited

The Distance and the near-IR extinction of the Monoceros Supernova Remnant

H. Zhao, B. W. Jiang, S. Gao +2

Supernova remnants (SNRs) embody the information of the influence on dust properties by the supernova explosion. Based on the color indexes from the 2MASS photometric survey and th…

astro-ph.GA2017★ 25 cited

The Optical -- Mid-infrared Extinction Law of the l=165 Sightline in the Galactic Plane: Diversity of Extinction Law in the Diffuse Interstellar Medium

Shu Wang, Biwei Jiang, He Zhao +2

Understanding the effects of dust extinction is important to properly interpret observations. The optical total-to-selective extinction ratio, Rv = Av/E(B-V), is widely used to des…