Exploring the correlation between Hα-to-UV ratio and burstiness for typical star-forming galaxies at z ∼ 2
The-to-UV luminosity ratio () is often used to probe bursty star formation histories (SFHs) of
star-forming galaxies and it is important to validate it against other proxies for burstiness. To …
star-forming galaxies and it is important to validate it against other proxies for burstiness. To …
A multiwavelength study of star formation in nearby galaxies: evidence for inside-out growth of the stellar disc
Global, radial, and local photometric measurements of several nearby low-mass galaxies
are presented. Multiwavelength observations are used to trace the distributions of old and …
are presented. Multiwavelength observations are used to trace the distributions of old and …
FAST discovery of an extra plume in DDO 168
NP Yu, M Zhu, JL Xu, CP Zhang, XL Liu… - Monthly Notices of …, 2023 - academic.oup.com
With the aim to study the extended H i environment around dwarf galaxies in the local
universe, we performed a high-sensitivity H i observation of the DDO 168 and DDO 167 pair …
universe, we performed a high-sensitivity H i observation of the DDO 168 and DDO 167 pair …
A comparative study of star-forming dwarf galaxies using the UVIT
S Amrutha, M Das, J Yadav - Monthly Notices of the Royal …, 2024 - academic.oup.com
We present a far-ultraviolet (FUV) study of 16 star-forming dwarf galaxies (SFDGs) using the
Ultra Violet Imaging Telescope. Morphologically, SFDGs are classified as dwarf spirals …
Ultra Violet Imaging Telescope. Morphologically, SFDGs are classified as dwarf spirals …
The growth history of local M 33-mass bulgeless spiral galaxies
X Kang, RP Kudritzki, F Zhang - Astronomy & Astrophysics, 2023 - aanda.org
NGC 7793, NGC 300, M 33, and NGC 2403 are four nearby undisturbed and bulgeless low-
mass spiral galaxies whose morphology and stellar mass are similar. They are ideal …
mass spiral galaxies whose morphology and stellar mass are similar. They are ideal …
A multiwavelength study of nearby star-forming spiral galaxies and the clustering of star formation in M63
This multiwavelength study of the star formation and star formation history (SFH) trends in
the nearby universe looks at nine nearby late-type spirals. Spectral energy distributions fitted …
the nearby universe looks at nine nearby late-type spirals. Spectral energy distributions fitted …
No Evidence of a Correlation between -to-UV Ratio and Burstiness for Typical Star-forming Galaxies at
S Rezaee, NA Reddy, MW Topping, I Shivaei… - arXiv preprint arXiv …, 2022 - arxiv.org
It has long been uncertain how effective the dust-corrected H $\alpha $-to-UV luminosity
ratio ($ L (\rm H\alpha)/L (\rm UV) $) is in probing bursty SFHs for high-redshift galaxies. To …
ratio ($ L (\rm H\alpha)/L (\rm UV) $) is in probing bursty SFHs for high-redshift galaxies. To …
[PDF][PDF] No Evidence of a Correlation between Hα-to-UV Ratio and Burstiness for Typical Star-forming Galaxies at z∼ 2
NA Reddy, MW Topping, I Shivaei, AE Shapley… - Monthly notices of the …, 2023 - par.nsf.gov
It has long been uncertain how effective the dust-corrected H𝛼-to-UV luminosity ratio (𝐿
(H𝛼)/𝐿 (UV)) is in probing bursty star-formation histories (SFHs) for high-redshift galaxies …
(H𝛼)/𝐿 (UV)) is in probing bursty star-formation histories (SFHs) for high-redshift galaxies …
Studying Global and Local Star Formation Processes with Young Massive Stars in NGC 6946
D Tran - 2024 - search.proquest.com
I analyze resolved near-ultraviolet (NUV) stellar photometry of star-forming galaxy NGC
6946 (The Fireworks Galaxy) taken with the Hubble Space Telescope's (HST) Wide Field …
6946 (The Fireworks Galaxy) taken with the Hubble Space Telescope's (HST) Wide Field …
Variation of the Nebular and Stellar Dust Attenuation Curve With Physical Properties of Local and High-Redshift Star-Forming Galaxies
S Rezaee - 2023 - search.proquest.com
Dust attenuation refers to the absorption and scattering of light by interstellar dust particles
within a galaxy. This effect, which depends on wavelength, is also known as dust reddening …
within a galaxy. This effect, which depends on wavelength, is also known as dust reddening …