Results 121 to 130 of about 14,171 (214)

Role of gibberellins, neem leaf extract, and serine in improving wheat growth and grain yield under drought-triggered oxidative stress. [PDF]

Physiol Mol Biol Plants, 2023
Hameed S, Atif M, Perveen S.
europepmc   +1 more source

Active Galactic Nuclei in the Green Valley at z ∼ 0.7

The Astrophysical Journal
We present near-infrared (NIR) spectroscopy using the MMT and Magellan infrared spectrograph for a sample of 29 massive galaxies ( $\mathrm{log}\ {M}_{* }/{M}_{\odot }\gtrsim 10$ ) at z ∼ 0.7 with optical spectroscopy from the Large Early Galaxy ...
Charity Woodrum, Christina C. Williams, Marcia Rieke, Kevin N. Hainline, Raphael E. Hviding, Zhiyuan Ji, Robert Kennicutt, Christopher N. A. Willmer   +7 more
doaj   +1 more source

The cumulative star formation histories of dwarf galaxies with TNG50. I: environment-driven diversity and connection to quenching [PDF]

, 2021
Gandhali D Joshi, Annalisa Pillepich, Dylan Nelson, Elad Zinger, Federico Marinacci, Volker Springel, Mark Vogelsberger, Lars Hernquist   +7 more
openalex   +1 more source

Investigating Galaxy Quenching With The Sdss: Stellar Metallicities As A Tracer Of Quenching Mechanisms

, 2017
Peng et al. (2015, Nature, 521, 192) analysed stellar metallicities of 26,000 SDSS galaxies and found that galaxies with stellar masses below 1011 solar masses are primarily quenched due to the halting of the supply of cold gas (strangulation). We take this analysis further by making use of the much larger spectroscopic sample of galaxies in SDSS DR7 ...
Daniel Thomas, Roberto Maiolino, Claudia Maraston, James Trussler, Daniel Goddard, Yingjie Peng   +5 more
openaire   +2 more sources

Galaxy evolution in the post-merger regime. II -- Post-merger quenching peaks within 500 Myr of coalescence

The Open Journal of Astrophysics
Mechanisms for quenching star formation in galaxies remain hotly debated, with galaxy mergers an oft-proposed pathway. In Ellison et al. (2022) we tested this scenario by quantifying the fraction of recently and rapidly quenched post-starbursts (PSBs) in
Sara Ellison, Leonardo Ferreira, Vivienne Wild, Scott Wilkinson, Kate Rowlands, David R. Patton   +5 more
doaj   +1 more source

Improved SED-fitting Assumptions Result in Inside-out Quenching at z ~ 0.5 and Quenching at All Radii Simultaneously at z ~ 1

The Astrophysical Journal
Many studies conclude that galaxies quench from the inside-out by examining profiles of specific star formation rate (sSFR). These are usually measured by fitting spectral energy distributions (SEDs) assuming a fixed dust law and uniform priors on all ...
Alexander de la Vega, Susan A. Kassin, Camilla Pacifici, Stéphane Charlot, Emma Curtis-Lake, Jacopo Chevallard, Timothy M. Heckman, Anton M. Koekemoer, Weichen Wang   +8 more
doaj   +1 more source

What is the right way to quench star formation in semi-analytic models of galaxy formation? [PDF]

, 2017
Yu Luo, Xi Kang
openalex   +1 more source

Assessment of SDSS-derived Galaxy Morphologies Using HST Imaging

The Astrophysical Journal
The Sloan Digital Sky Survey (SDSS) was foundational to the study of galaxy evolution, having revealed the bimodality of galaxies and the relationship between their structure and star-forming activity.
Chandler Osborne, Samir Salim
doaj   +1 more source

Connection between Stellar Mass Distributions within Galaxies and Quenching Since z = 2 [PDF]

, 2017
Moein Mosleh, Sandro Tacchella, A. Renzini, C. M. Carollo, Alireza Molaeinezhad, Masato Onodera, Habib G. Khosroshahi, S. J. Lilly   +7 more
openalex   +1 more source

A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters [PDF]

, 2020
Kyle A. Oman, Yannick M. Bahé, J. Healy, Kelley M. Hess, Michael J. Hudson, Marc Verheijen   +5 more
openalex   +1 more source