Starburst Galaxy
SOFIA/HAWC+ Detection of a Gravitationally Lensed Starburst Galaxy at z = 1 03
... lensed starburst galaxy HATLASJ1429-0028 (also known as ...disk galaxy at z = ...infrared galaxy at z = ...distant galaxy studies including the decomposition of SF/AGN components, which ...
8
Broadband Millimeter-Wave Spectroscopy with Z-Spec: An Unbiased Molecular-Line Survey of the Starburst Galaxy M82
... prototypical starburst galaxy and an ideal candidate for investigating physical conditions present in galaxies with large quantities of dust and molecular gas and undergoing rapid star ...nuclear ...
174
Dense Molecular Gas Tracers in the Outflow of the Starburst Galaxy NGC 253
... nearby starburst galaxy NGC 253 using ...central starburst region of NGC 253 and other starburst ...the starburst, and that its physical state does not change signi fi cantly over ...
10
CIRPASS near-infrared integral-field spectroscopy of massive star clusters in the starburst galaxy NGC 1140
... the starburst event responsible for the formation of the NGC 1140 YMCs indeed induced (compact) YMC formation on a galaxy-wide scale on short time-scales, and would thereby simultaneously cause significant ...
15
Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA
... and 1.0 mm, respectively) and CO (5–4) flux and velocity, created by S15, using the lensing model by Dye et al. (2015). This model was used in the image plane with the semilinear inversion method (Warren & Dye 2003) ...
11
Observations of carbon monoxide in the starburst galaxy M82 with a 690 GHz wide spectral bandwidth receiver
... observe an entire emission line with a single receiver tuning. The second part of this thesis describes the development of a 4-8 GHz low-noise amplifier (LNA) for use in the 690 GHz galaxy receiver. Microwave ...
187
Evolution of starburst galaxies in the Illustris simulation
... pre-merger/harassment starburst sample) have a neighbour with a stellar mass at least 10% that of the starburst ...pre-merger/harassment starburst galaxies, there are no surrounding galaxies or ...a ...
11
Herschel reveals the obscured star formation in HiZELS Hα emitters at z=1.47
... Figure 2. The stacked far-IR flux densities obtained for different HiZELS samples at z = 1.47. Photometry points come from Spitzer (24 and 70 μ m), Herschel (100, 160, 250, 350 and 500 μ m) and AzTEC (1100 μ m) images ...
18
Evolution of the cold gas properties of simulated post starburst galaxies
... agreement with those seen in observational samples. The simulation reproduces the observed time evolution of the gas fraction of the post-starburst galaxy population, with the average galaxy losing ≈ ...
15
The Evolutionary Sequence of Post Starburst Galaxies
... post-starburst galaxy that were identi- fied by Dressler & Gunn (1983) as having an elliptical morphology but rich in A-class ...recent starburst approximately 1-3 Gyr ago, that has been quenched ...
11
Causing a stir : radiative and mechanical feedback in starburst galaxies
... infrared galaxy was NGC 6240 (Zasov & Karachentsev 1979), and many more followed with observations from the InfraRed Astronomical Satellite (IRAS), which was launched in 1983 (Houck et ...merging galaxy ...
188
The diverse evolutionary pathways of post starburst galaxies
... powerful starburst and subsequent decline in SFR (ID17473042 and ...the galaxy either back to the blue cloud with decreased sSFR (ID9052812) or near/onto the red sequence (ID17473042), depending on the ...
11
The origins of post starburst galaxies at z < 0 05
... As well as their very broad distribution of n, covering both star-forming and quiescent control samples, the ePSB galaxies also show on average a higher fraction of stellar mass formed in the recent past than the ...
38
The properties of post starburst galaxies from spectral fitting
... With UDS we limit ourselves to discussion more by combining with other work, we may be able to tackle the results from UDS and UDSz in the future. Clearly all galaxies z ∼ 1 have formed a large fraction of mass in the ...
127
The case for two-dimensional galaxy–galaxy lensing
... the galaxy grouping information that would accurately clas- sify the galaxies as centrals and satellites (Hoekstra 2014) as it was realised that these objects need to be modelled sepa- ...the galaxy ...
9
KiDS-450: tomographic cross-correlation of galaxy shear with Planck lensing
... the galaxy intrinsic alignments, from residual systematic bias in the shear mul- tiplicative term m (equation 7), from astrophysical phenomena such as massive neutrinos and/or baryonic feedback, and from residual ...
15
On the galaxy-halo connection in the EAGLE simulation
... than in the SHAM+MMW model, and close to the predictions of SHAM alone. We show the success of EAGLE over SHAM + MMW to be due not to differences in underlying halo properties caused by baryons (Section 3.2), but rather ...
5
Unveiling galaxy bias via the halo model, KiDS, and GAMA
... The same issue occurs in the write-up in several earlier publications of our KiDS team. For example, the equations (2,5,6) in Viola et al. (2015) show this inconsistency (where we also point out a typo in the integration ...
21
The evolution of the cold interstellar medium in galaxies following a starburst
... central starburst has been identified through 3 arcsec fibre spectroscopy, it is possible that the lack of change in the molecular gas-to-stellar mass ratio may be because the central starburst does not ...
22
Surface Photometry of Spiral Galaxy NGC 5005 and Elliptical Galaxy NGC 4278 Zahraa Adnan| Abdullah K. Ahmed
... Spiral barred galaxy NGC 5005 is an inclined SAB(rs)bc Seyfert, at a distance of D = 16.9±6.7 Mpc, with a broad-line LINER (low- ionization nuclear emission line regions) nucleus(1, 2), this system is clearly ...
10