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galaxies: starburst

Massive post starburst galaxies at z > 1 are compact proto spheroids

Massive post starburst galaxies at z > 1 are compact proto spheroids

... distant galaxies and their structural ...(PSB) galaxies, which are observed a few hundred Myr after a major episode of star forma- tion was rapidly ...red-sequence” galaxies using rest-frame UVJ ...

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The properties of post starburst galaxies from spectral fitting

The properties of post starburst galaxies from spectral fitting

... post- starburst galaxies are consistent with being gas rich star-forming ...the starburst may or may not alter the galaxy morphology to be elliptical, as many of the PSB galaxies have disky ...

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The evolution of post starburst galaxies from z=2 to 0 5

The evolution of post starburst galaxies from z=2 to 0 5

... PSB galaxies compared to spectroscopic searches is diffi- cult to ascertain without large, blind spectroscopic surveys for ...post-starburst galaxies detected in the spectroscopic BOSS survey by ...

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The evolution of the cold interstellar medium in galaxies following a starburst

The evolution of the cold interstellar medium in galaxies following a starburst

... 0.03 starburst to post-starburst (PSB) galaxies selected to span an age sequence from ongoing starburst to 1 Gyr after the starburst ...the starburst due to exhaustion or ...

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The origins of post starburst galaxies at z < 0 05

The origins of post starburst galaxies at z < 0 05

... post-starburst galaxies in which the star-formation has effectively been quenched, selected based on the lack of measurable nebular emission, usually the [OII] line ...a starburst is not an ...

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The structure of post starburst galaxies at 0 5 < z < 2: evidence for two distinct quenching routes at different epochs

The structure of post starburst galaxies at 0 5 < z < 2: evidence for two distinct quenching routes at different epochs

... At low redshift ( z < 0.1), gas-rich major mergers have also been linked to PSBs in low-density environments (e.g. Zabludoff et al. 1996; Blake et al. 2004; Pawlik et al. 2016, 2018). However, in contrast to our ...

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Post starburst galaxies in SDSS IV MaNGA

Post starburst galaxies in SDSS IV MaNGA

... control galaxies again suggests a recent strong inflow of gas to the central ...RPSB galaxies have not (yet) suffered global quenching of the star ...a starburst and cause post-starburst ...

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Evolution of the cold gas properties of simulated post starburst galaxies

Evolution of the cold gas properties of simulated post starburst galaxies

... field galaxies and are thought to play a role in triggering the starbursts that initiate the formation of PSBs ...extreme starburst, but also by the loss of gas in other ways, for instances in triggered AGN ...

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The origin and fate of post starburst galaxies : morphological and structural image analysis of local galaxies with recent episodes of enhanced star formation

The origin and fate of post starburst galaxies : morphological and structural image analysis of local galaxies with recent episodes of enhanced star formation

... central starburst dominates the bulges in the low-mass galaxies but the same is not true in the case of the most massive systems, which could mean that the fractions of stellar mass formed during the ...

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Massive post starburst galaxies at z > 1 are compact proto spheroids

Massive post starburst galaxies at z > 1 are compact proto spheroids

... distant galaxies and their structural ...(PSB) galaxies, which are observed a few hundred million years after a major episode of star formation was rapidly ...sequence’ galaxies using rest-frame UVJ ...

12

The evolution of post starburst galaxies from z=2 to 0 5

The evolution of post starburst galaxies from z=2 to 0 5

... of galaxies in star formation rate/stellar mass/morphology planes can only help to constrain the role of different processes in shutting down star formation in combination with detailed models which help to link ...

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Starburst galaxies in the COSMOS field : clumpy star formation at redshift 0 < z

Starburst galaxies in the COSMOS field : clumpy star formation at redshift 0 < z <0 5

... galaxies (obtained from the Sloan Digital Sky Survey; SDSS) massive clumps in local starbursts belonging to the Kiso Sur- vey (Miyauchi-Isobe et al. 2010), and clumps in galaxies at high redshift from the ...

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The role of massive stars in young starburst galaxies

The role of massive stars in young starburst galaxies

... tarburst galaxies are defined ais those galaxies undergoing violent star formation over relatively short periods of time (10 to 100 M yr), These objects may form stellar popula­ tions of greater than 10^ ...

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The Evolutionary Sequence of Post Starburst Galaxies

The Evolutionary Sequence of Post Starburst Galaxies

... post-starburst galaxies. After the initial starburst has ended the galaxies are seen as blue spirals/disks with a young stellar spectra, indicated by deep Balmer absorption ...disk ...

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The structure of post starburst galaxies at 0 5 < z < 2 : evidence for two distinct quenching routes at different epochs

The structure of post starburst galaxies at 0 5 < z < 2 : evidence for two distinct quenching routes at different epochs

... At low redshift (z < 0.1), gas-rich major mergers have also been linked to PSBs in low-density environments (e.g. Zabludoff et al. 1996; Blake et al. 2004; Pawlik et al. 2016, 2018). However, in contrast to our ...

21

Evolution of starburst galaxies in the Illustris simulation

Evolution of starburst galaxies in the Illustris simulation

... a starburst, we find in this study, that harassment events can also trigger a starburst that is comparable in ...rounding galaxies to test directly whether harassments are the main trigger for the ...

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The diverse evolutionary pathways of post starburst galaxies

The diverse evolutionary pathways of post starburst galaxies

... Simulated galaxies in the z = ...two galaxies can cause a powerful starburst and subsequent decline in SFR (ID17473042 and ...post-starburst galaxies with no visible signs of ...

11

Revealing the differences in the SMBH accretion rate distributions of starburst and non-starburst galaxies

Revealing the differences in the SMBH accretion rate distributions of starburst and non-starburst galaxies

... At face value, our results seem to show no indica- tion that intense radiation produced from an AGN dur- ing an accretion phase negatively impacts star-formation (Di Matteo et al. 2005; Fabian 2012). Otherwise, we may ...

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CIRPASS near-infrared integral-field spectroscopy of massive star clusters in the starburst galaxy NGC 1140

CIRPASS near-infrared integral-field spectroscopy of massive star clusters in the starburst galaxy NGC 1140

... It appears, therefore, that there may be a small age gradient from complex [H94a]1–3 to complex [H94a]6–7. Although we justified our assumption of a mean YMC metallicity of 0.4 Z ⊙ in Section 4.1, we also performed our ...

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Diagnostics of a nuclear starburst: water and methanol masers

Diagnostics of a nuclear starburst: water and methanol masers

... star-forming galaxies, ...2015). Starburst driven winds are a result of feedback in the form of supernovae and stellar winds ...nuclear starburst of the nearby galaxy NGC 253 using astrophysical H 2 ...

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