Multiple mechanisms quench passive spiral galaxies

QR Code

Multiple mechanisms quench passive spiral galaxies

We examine the properties of a sample of 35 nearby passive spiral galaxies in order to determine their dominant quenching mechanism(s). All five low-mass (M⋆ < 1 × 1010 M⊙) passive spiral galaxies are located in the rich Virgo cluster. This is in contrast to low-mass spiral galaxies with star for...

Full description

Bibliographic Details
Main Authors:	Fraser-McKelvie, Amelia, Brown, Michael J. I., Pimbblet, Kevin, Dolley, Tim, Bonne, Nicolas J.
Format:	Article
Published:	Oxford University Press 2018
Subjects:	galaxies: evolution galaxies: general galaxies: spiral galaxies: stellar content
Online Access:	https://eprints.nottingham.ac.uk/50495/

Similar Items

Excavating the fossil record of spiral galaxies
by: Peterken, Thomas
Published: (2020)

SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment
by: Goddard, D., et al.
Published: (2017)

Galaxy and Mass Assembly (GAMA): morphological transformation of galaxies across the green valley
by: Bremer, M.N., et al.
Published: (2018)

SDSS-IV MaNGA: properties of galaxies with kinematically decoupled stellar and gaseous components
by: Jin, Yifei, et al.
Published: (2016)

Galaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband images
by: Kruk, Sandor J., et al.
Published: (2018)

Galaxy Zoo: constraining the origin of spiral arms
by: Hart, Ross E., et al.
Published: (2018)

Galaxy Zoo: star formation versus spiral arm number
by: Hart, Ross E., et al.
Published: (2017)

SDSS-IV MaNGA: bulge–disc decomposition of IFU data cubes (BUDDI)
by: Johnston, Evelyn J., et al.
Published: (2017)

P-MaNGA: gradients in recent star formation histories as diagnostics for galaxy growth and death
by: Li, Cheng, et al.
Published: (2015)

SDSS-IV MaNGA: star formation cessation in low-redshift galaxies I: dependence on stellar mass and structural properties
by: Wang, Enci, et al.
Published: (2018)

Galaxy Zoo: evidence for rapid, recent quenching within a population of AGN host galaxies
by: Smethurst, Rebecca J., et al.
Published: (2016)

The demographics of galactic bulges in the SDSS database
by: Kim, Keunho, et al.
Published: (2016)

The evolution of post-starburst galaxies from z=2 to 0.5
by: Wild, Vivienne, et al.
Published: (2016)

Galaxy Zoo: the interplay of quenching mechanisms in the group environment
by: Smethurst, Rebecca J., et al.
Published: (2017)

Galaxy Zoo: quantitative visual morphological classifications for 48 000 galaxies from CANDELS
by: Simmons, B.D., et al.
Published: (2017)

Galaxy Zoo and SPARCFIRE: constraints on spiral arm formation mechanisms from spiral arm number and pitch angles
by: Hart, Ross E., et al.
Published: (2017)

Galaxy Zoo: comparing the demographics of spiral arm number and a new method for correcting redshift bias
by: Hart, Ross E., et al.
Published: (2016)

The origin of S0s in clusters: evidence from the bulge and disc star formation histories
by: Johnston, Evelyn J., et al.
Published: (2014)

The effect of the environment on the structure, morphology and star-formation history of intermediate-redshift galaxies
by: Kelkar, Kshitija, et al.
Published: (2017)

The identification of post-starburst galaxies at z∼1 using multiwavelength photometry: a spectroscopic verification
by: Maltby, David T., et al.
Published: (2016)

Galaxy Zoo: finding offset discs and bars in SDSS galaxies
by: Kruk, Sandor J., et al.
Published: (2017)

The evolution of galaxies at constant number density: a less biased view of star formation, quenching, and structural formation
by: Ownsworth, Jamie R., et al.
Published: (2016)

Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey
by: Kelkar, K., et al.
Published: (2015)

The Evolution of Galaxies in Proto-clusters
by: Werner, Stephane V.
Published: (2023)

Resolving the disc–halo degeneracy – I: a look at NGC 628
by: Aniyan, S, et al.
Published: (2018)

Galaxy and Mass Assembly (GAMA): active galactic nuclei in pairs of galaxies
by: Gordon, Yjan A., et al.
Published: (2017)

The environmental dependence of the structure of galactic discs in STAGES S0 galaxies: implications for S0 formation
by: Maltby, David Terence, et al.
Published: (2015)

Herschel-ATLAS: the surprising diversity of dust-selected galaxies in the local submillimetre Universe
by: Clark, C.J.R., et al.
Published: (2015)

Semi-analytic model predictions of the galaxy population in protoclusters
by: Contini, E., et al.
Published: (2016)

Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s
by: Rodriguez Del Pino, Bruno, et al.
Published: (2014)

Galaxy evolution in protoclusters
by: Muldrew, Stuart I., et al.
Published: (2017)

Major merging history in CANDELS. I. Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0
by: Mantha, Kameswara Bharadwaj, et al.
Published: (2018)

Exploring the progenitors of brightest cluster galaxies at z ∼ 2
by: Zhao, Dongyao, et al.
Published: (2017)

Structural evolution of massive galaxies in the last 11 Gyr
by: Buitrago Alonso, Fernando
Published: (2012)

The Cosmic Chemical Evolution Histories of Spiral Galaxies
by: Greener, Michael John
Published: (2023)

The SCUBA-2 Cosmology Legacy Survey: multi-wavelength properties of ALMA-identified submillimeter galaxies in UKIDSS UDS
by: Simpson, J.M., et al.
Published: (2017)

The LOFAR window on star-forming galaxies and AGNs – curved radio SEDs and IR–radio correlation at 0<z<2.5
by: Calistro Rivera, G., et al.
Published: (2017)

The formation of bulges, discs and two-component galaxies in the CANDELS Survey at z < 3
by: Margalef-Bentabol, Berta, et al.
Published: (2016)

Stellar populations, stellar masses and the formation of galaxy bulges and discs at z < 3 in CANDELS
by: Margalef-Bentabol, Berta, et al.
Published: (2018)

Clumpy galaxies in CANDELS. II. Physical properties of UV-bright clumps at 0.5 ≤ z < 3
by: Guo, Yicheng, et al.
Published: (2018)