FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2014753653> ?p ?o ?g. }

• W2014753653 endingPage "43" @default.
• W2014753653 startingPage "43" @default.
• W2014753653 abstract "(Abridged) We analyze the environments and galactic properties (morphologies and star-formation histories) of a sample of 153 close kinematic pairs in the redshift range 0.2 < z < 1 identified in the zCOSMOS-bright 10k spectroscopic sample of galaxies. Correcting for projection effects, the fraction of close kinematic pairs is three times higher in the top density quartile than in the lowest one. This translates to a three times higher merger rate because the merger timescales are shown, from mock catalogues based on the Millennium simulation, to be largely independent of environment once the same corrections for projection is applied. We then examine the morphologies and stellar populations of galaxies in the pairs, comparing them to control samples that are carefully matched in environment so as to remove as much as possible the well-known effects of environment on the properties of the parent population of galaxies. Once the environment is properly taken into account in this way, we find that the early-late morphology mix is the same as for the parent population, but that the fraction of irregular galaxies is boosted by 50-75%, with a disproportionate increase in the number of irregular-irregular pairs (factor of 4-8 times), due to the disturbance of disk galaxies. Future dry-mergers, involving elliptical galaxies comprise less than 5% of all close kinematic pairs. In the closest pairs, there is a boost in the specific star-formation rates of star-forming galaxies of a factor of 2-4, and there is also evidence for an increased incidence of post star-burst galaxies. Although significant for the galaxies involved, the excess star-formation associated with pairs represents only about 5% of the integrated star-formation activity in the parent sample. Although most pair galaxies are in dense environments, the effects of interaction appear to be largest in the lower density environments." @default.
• W2014753653 created "2016-06-24" @default.
• W2014753653 creator A5001219575 @default.
• W2014753653 creator A5001328043 @default.
• W2014753653 creator A5004193106 @default.
• W2014753653 creator A5007647078 @default.
• W2014753653 creator A5009404806 @default.
• W2014753653 creator A5009428303 @default.
• W2014753653 creator A5012431420 @default.
• W2014753653 creator A5015975135 @default.
• W2014753653 creator A5019699312 @default.
• W2014753653 creator A5021267951 @default.
• W2014753653 creator A5021288660 @default.
• W2014753653 creator A5022137696 @default.
• W2014753653 creator A5022894838 @default.
• W2014753653 creator A5023265038 @default.
• W2014753653 creator A5023314136 @default.
• W2014753653 creator A5024335460 @default.
• W2014753653 creator A5026007485 @default.
• W2014753653 creator A5028548201 @default.
• W2014753653 creator A5029867699 @default.
• W2014753653 creator A5030920057 @default.
• W2014753653 creator A5031242872 @default.
• W2014753653 creator A5034718849 @default.
• W2014753653 creator A5035438463 @default.
• W2014753653 creator A5035540139 @default.
• W2014753653 creator A5036504183 @default.
• W2014753653 creator A5037658542 @default.
• W2014753653 creator A5041408764 @default.
• W2014753653 creator A5043022402 @default.
• W2014753653 creator A5043083140 @default.
• W2014753653 creator A5048044337 @default.
• W2014753653 creator A5048538677 @default.
• W2014753653 creator A5051323119 @default.
• W2014753653 creator A5056456679 @default.
• W2014753653 creator A5056788425 @default.
• W2014753653 creator A5059163525 @default.
• W2014753653 creator A5061217737 @default.
• W2014753653 creator A5061935397 @default.
• W2014753653 creator A5066116709 @default.
• W2014753653 creator A5066433728 @default.
• W2014753653 creator A5067616980 @default.
• W2014753653 creator A5068797292 @default.
• W2014753653 creator A5069101046 @default.
• W2014753653 creator A5070004095 @default.
• W2014753653 creator A5072069478 @default.
• W2014753653 creator A5073025095 @default.
• W2014753653 creator A5075023487 @default.
• W2014753653 creator A5075132871 @default.
• W2014753653 creator A5078337785 @default.
• W2014753653 creator A5081204604 @default.
• W2014753653 creator A5085036611 @default.
• W2014753653 creator A5085221278 @default.
• W2014753653 creator A5085738019 @default.
• W2014753653 creator A5086020534 @default.
• W2014753653 creator A5088219275 @default.
• W2014753653 creator A5089515217 @default.
• W2014753653 creator A5089583649 @default.
• W2014753653 creator A5089668675 @default.
• W2014753653 creator A5090420192 @default.
• W2014753653 creator A5090824172 @default.
• W2014753653 date "2012-12-14" @default.
• W2014753653 modified "2023-10-18" @default.
• W2014753653 title "ENVIRONMENTAL EFFECTS IN THE INTERACTION AND MERGING OF GALAXIES IN zCOSMOS" @default.
• W2014753653 cites W1967063442 @default.
• W2014753653 cites W1970529252 @default.
• W2014753653 cites W1972763344 @default.
• W2014753653 cites W1973275093 @default.
• W2014753653 cites W1973759546 @default.
• W2014753653 cites W1979423107 @default.
• W2014753653 cites W1982717117 @default.
• W2014753653 cites W1984328214 @default.
• W2014753653 cites W1984389533 @default.
• W2014753653 cites W1984644267 @default.
• W2014753653 cites W1985952407 @default.
• W2014753653 cites W1986761806 @default.
• W2014753653 cites W1989738732 @default.
• W2014753653 cites W1993749637 @default.
• W2014753653 cites W1993839984 @default.
• W2014753653 cites W1995641972 @default.
• W2014753653 cites W1995667613 @default.
• W2014753653 cites W1997529816 @default.
• W2014753653 cites W1999793606 @default.
• W2014753653 cites W2000685740 @default.
• W2014753653 cites W2001717952 @default.
• W2014753653 cites W2007325934 @default.
• W2014753653 cites W2007335458 @default.
• W2014753653 cites W2007608095 @default.
• W2014753653 cites W2011193914 @default.
• W2014753653 cites W2020478543 @default.
• W2014753653 cites W2021721029 @default.
• W2014753653 cites W2033227485 @default.
• W2014753653 cites W2033539580 @default.
• W2014753653 cites W2033648059 @default.
• W2014753653 cites W2046620005 @default.
• W2014753653 cites W2047688075 @default.
• W2014753653 cites W2052755662 @default.
• W2014753653 cites W2055327934 @default.

• next