Matches in SemOpenAlex for { <https://semopenalex.org/work/W2001669642> ?p ?o ?g. }
- W2001669642 endingPage "433" @default.
- W2001669642 startingPage "419" @default.
- W2001669642 abstract "We present a stellar population synthesis study of a type II luminous infrared galaxy, IRASF21013-0739. Optical images show clear characteristics of a merger remnant. The H-band absolute magnitude is MH = −25.1, which is ∼2 times as luminous as L* galaxies. Stellar populations are obtained through the stellar synthesis code STARLIGHT. We find that it experienced a recent starburst (SB) phase ∼ 100 Myr ago. By reconstructing the ultraviolet-to-optical spectrum, and adopting Calzetti et al. and Leitherer et al.'s extinction curves, we estimate the past infrared (IR) luminosities of the host galaxy and find it may have experienced an ultraluminous infrared galaxy phase which lasted for about 100 Myr. Its i-band absolute magnitude is Mi = −22.463, and its spectral type shows type 2 active galactic nucleus (AGN) characteristics. The mass of the supermassive black-hole is estimated to be MBH = 1.6 × 107 M⊙ (lower-limit). The Eddington ratio Lbol/LEdd is 0.15, which is typical of Palomar-Green (PG) quasars. Both the nuclear SB and AGN contribute to the present IR luminosity budget, and the SB contributes ∼67%. On the diagram of IR color versus IR/optical excess, it is located between IR quasars and PG quasars. These results indicate that IRASF21013-0739 has probably evolved from a ULIRG, and it can possibly evolve into an AGN." @default.
- W2001669642 created "2016-06-24" @default.
- W2001669642 creator A5002615106 @default.
- W2001669642 creator A5020798050 @default.
- W2001669642 creator A5066340187 @default.
- W2001669642 date "2011-03-25" @default.
- W2001669642 modified "2023-09-26" @default.
- W2001669642 title "IRAS F21013-0739: a possible evolutionary successor of an ultraluminous infrared galaxy" @default.
- W2001669642 cites W1520068934 @default.
- W2001669642 cites W1847269195 @default.
- W2001669642 cites W1964921686 @default.
- W2001669642 cites W1972815068 @default.
- W2001669642 cites W1978188520 @default.
- W2001669642 cites W1979115990 @default.
- W2001669642 cites W1983058503 @default.
- W2001669642 cites W1983961944 @default.
- W2001669642 cites W1987811751 @default.
- W2001669642 cites W1993355650 @default.
- W2001669642 cites W1993785188 @default.
- W2001669642 cites W1994671833 @default.
- W2001669642 cites W1994703407 @default.
- W2001669642 cites W1994718036 @default.
- W2001669642 cites W1995619964 @default.
- W2001669642 cites W1996024911 @default.
- W2001669642 cites W1999299181 @default.
- W2001669642 cites W2007790517 @default.
- W2001669642 cites W2011875707 @default.
- W2001669642 cites W2018489450 @default.
- W2001669642 cites W2018858432 @default.
- W2001669642 cites W2019274267 @default.
- W2001669642 cites W2023267266 @default.
- W2001669642 cites W2027862338 @default.
- W2001669642 cites W2030410680 @default.
- W2001669642 cites W2031203855 @default.
- W2001669642 cites W2035945931 @default.
- W2001669642 cites W2038082407 @default.
- W2001669642 cites W2038680891 @default.
- W2001669642 cites W2053658940 @default.
- W2001669642 cites W2054026519 @default.
- W2001669642 cites W2056085571 @default.
- W2001669642 cites W2058890501 @default.
- W2001669642 cites W2058947019 @default.
- W2001669642 cites W2059836646 @default.
- W2001669642 cites W2061710077 @default.
- W2001669642 cites W2063903220 @default.
- W2001669642 cites W2069771108 @default.
- W2001669642 cites W2069847092 @default.
- W2001669642 cites W2073285288 @default.
- W2001669642 cites W2076566856 @default.
- W2001669642 cites W2077326407 @default.
- W2001669642 cites W2077625084 @default.
- W2001669642 cites W2079854010 @default.
- W2001669642 cites W2080259687 @default.
- W2001669642 cites W2084098739 @default.
- W2001669642 cites W2084674774 @default.
- W2001669642 cites W2085780075 @default.
- W2001669642 cites W2089960678 @default.
- W2001669642 cites W2090268762 @default.
- W2001669642 cites W2090395333 @default.
- W2001669642 cites W2094973357 @default.
- W2001669642 cites W2111817932 @default.
- W2001669642 cites W2112028701 @default.
- W2001669642 cites W2114791595 @default.
- W2001669642 cites W2115032180 @default.
- W2001669642 cites W2115234254 @default.
- W2001669642 cites W2124219338 @default.
- W2001669642 cites W2125083906 @default.
- W2001669642 cites W2131801207 @default.
- W2001669642 cites W2136466740 @default.
- W2001669642 cites W2143598938 @default.
- W2001669642 cites W2145451842 @default.
- W2001669642 cites W2151062050 @default.
- W2001669642 cites W2151684988 @default.
- W2001669642 cites W2155122056 @default.
- W2001669642 cites W2155475085 @default.
- W2001669642 cites W2602693422 @default.
- W2001669642 cites W3098153900 @default.
- W2001669642 cites W3098637484 @default.
- W2001669642 cites W3100231503 @default.
- W2001669642 cites W3100869364 @default.
- W2001669642 cites W3101550526 @default.
- W2001669642 cites W3103868583 @default.
- W2001669642 cites W3103994273 @default.
- W2001669642 cites W3104422960 @default.
- W2001669642 cites W3105105183 @default.
- W2001669642 cites W3106190097 @default.
- W2001669642 cites W3122565141 @default.
- W2001669642 cites W3122966038 @default.
- W2001669642 cites W3125484636 @default.
- W2001669642 cites W4240963171 @default.
- W2001669642 cites W4244818491 @default.
- W2001669642 cites W4300902987 @default.
- W2001669642 doi "https://doi.org/10.1088/1674-4527/11/4/005" @default.
- W2001669642 hasPublicationYear "2011" @default.
- W2001669642 type Work @default.
- W2001669642 sameAs 2001669642 @default.
- W2001669642 citedByCount "0" @default.
- W2001669642 crossrefType "journal-article" @default.