Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band)

In this project we analyze data of a large sample of gas rich dwarfs galaxies including; Low Surface Brightness Galaxies (LSBGs), Blue Compact Galaxies (BCGs), and dwarfs Irregulars (dIr). We then study the difference between properties of these galaxies in the range of radio frequencies (B-band...
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Autor*in:	Layali Y. Al-Mashhadani [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2017

Schlagwörter:	galaxies, Low Surface Brightness Galaxies, galaxies evolution, gas rich galaxies

Übergeordnetes Werk:	In: Ibn Al-Haitham Journal for Pure and Applied Sciences - University of Baghdad, 2019, 26(2017), 2
Übergeordnetes Werk:	volume:26 ; year:2017 ; number:2

Links:	Link aufrufen Link aufrufen Journal toc Journal toc

Katalog-ID:	DOAJ044856547

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spelling	(DE-627)DOAJ044856547 (DE-599)DOAJea66cc69b4b14ae8892556fe11c72a83 DE-627 ger DE-627 rakwb eng Layali Y. Al-Mashhadani verfasserin aut Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band) 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this project we analyze data of a large sample of gas rich dwarfs galaxies including; Low Surface Brightness Galaxies (LSBGs), Blue Compact Galaxies (BCGs), and dwarfs Irregulars (dIr). We then study the difference between properties of these galaxies in the range of radio frequencies (B-band). The data are available in HIPASS catalogue and McGaughâ€™s Data Page. We depended also NASA/IPACExtragalactic Databes web site http://ned.ipac.caltech.edu in the data reduction. We measured the gas evolution (HI mass), gas mass-to-luminosity ratio, and abundance of the elements such as the oxygen abundance for these galaxies. Our results show a big discrepancy between the behavior of LSBGs at low and high luminosity ranges. We find that the LSBGs have higher HI masses than other samples of BCGs. BCGs are forced to stem from LSBGs or from dlrs according to their gas to light ratio vs total luminosity value galaxies, Low Surface Brightness Galaxies, galaxies evolution, gas rich galaxies Science Q In Ibn Al-Haitham Journal for Pure and Applied Sciences University of Baghdad, 2019 26(2017), 2 (DE-627)756825806 (DE-600)2727526-7 25213407 nnns volume:26 year:2017 number:2 https://doaj.org/article/ea66cc69b4b14ae8892556fe11c72a83 kostenfrei https://jih.uobaghdad.edu.iq/index.php/j/article/view/484 kostenfrei https://doaj.org/toc/1609-4042 Journal toc kostenfrei https://doaj.org/toc/2521-3407 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 26 2017 2
allfields_unstemmed	(DE-627)DOAJ044856547 (DE-599)DOAJea66cc69b4b14ae8892556fe11c72a83 DE-627 ger DE-627 rakwb eng Layali Y. Al-Mashhadani verfasserin aut Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band) 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this project we analyze data of a large sample of gas rich dwarfs galaxies including; Low Surface Brightness Galaxies (LSBGs), Blue Compact Galaxies (BCGs), and dwarfs Irregulars (dIr). We then study the difference between properties of these galaxies in the range of radio frequencies (B-band). The data are available in HIPASS catalogue and McGaughâ€™s Data Page. We depended also NASA/IPACExtragalactic Databes web site http://ned.ipac.caltech.edu in the data reduction. We measured the gas evolution (HI mass), gas mass-to-luminosity ratio, and abundance of the elements such as the oxygen abundance for these galaxies. Our results show a big discrepancy between the behavior of LSBGs at low and high luminosity ranges. We find that the LSBGs have higher HI masses than other samples of BCGs. BCGs are forced to stem from LSBGs or from dlrs according to their gas to light ratio vs total luminosity value galaxies, Low Surface Brightness Galaxies, galaxies evolution, gas rich galaxies Science Q In Ibn Al-Haitham Journal for Pure and Applied Sciences University of Baghdad, 2019 26(2017), 2 (DE-627)756825806 (DE-600)2727526-7 25213407 nnns volume:26 year:2017 number:2 https://doaj.org/article/ea66cc69b4b14ae8892556fe11c72a83 kostenfrei https://jih.uobaghdad.edu.iq/index.php/j/article/view/484 kostenfrei https://doaj.org/toc/1609-4042 Journal toc kostenfrei https://doaj.org/toc/2521-3407 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 26 2017 2
allfieldsGer	(DE-627)DOAJ044856547 (DE-599)DOAJea66cc69b4b14ae8892556fe11c72a83 DE-627 ger DE-627 rakwb eng Layali Y. Al-Mashhadani verfasserin aut Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band) 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this project we analyze data of a large sample of gas rich dwarfs galaxies including; Low Surface Brightness Galaxies (LSBGs), Blue Compact Galaxies (BCGs), and dwarfs Irregulars (dIr). We then study the difference between properties of these galaxies in the range of radio frequencies (B-band). The data are available in HIPASS catalogue and McGaughâ€™s Data Page. We depended also NASA/IPACExtragalactic Databes web site http://ned.ipac.caltech.edu in the data reduction. We measured the gas evolution (HI mass), gas mass-to-luminosity ratio, and abundance of the elements such as the oxygen abundance for these galaxies. Our results show a big discrepancy between the behavior of LSBGs at low and high luminosity ranges. We find that the LSBGs have higher HI masses than other samples of BCGs. BCGs are forced to stem from LSBGs or from dlrs according to their gas to light ratio vs total luminosity value galaxies, Low Surface Brightness Galaxies, galaxies evolution, gas rich galaxies Science Q In Ibn Al-Haitham Journal for Pure and Applied Sciences University of Baghdad, 2019 26(2017), 2 (DE-627)756825806 (DE-600)2727526-7 25213407 nnns volume:26 year:2017 number:2 https://doaj.org/article/ea66cc69b4b14ae8892556fe11c72a83 kostenfrei https://jih.uobaghdad.edu.iq/index.php/j/article/view/484 kostenfrei https://doaj.org/toc/1609-4042 Journal toc kostenfrei https://doaj.org/toc/2521-3407 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 26 2017 2
allfieldsSound	(DE-627)DOAJ044856547 (DE-599)DOAJea66cc69b4b14ae8892556fe11c72a83 DE-627 ger DE-627 rakwb eng Layali Y. Al-Mashhadani verfasserin aut Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band) 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In this project we analyze data of a large sample of gas rich dwarfs galaxies including; Low Surface Brightness Galaxies (LSBGs), Blue Compact Galaxies (BCGs), and dwarfs Irregulars (dIr). We then study the difference between properties of these galaxies in the range of radio frequencies (B-band). The data are available in HIPASS catalogue and McGaughâ€™s Data Page. We depended also NASA/IPACExtragalactic Databes web site http://ned.ipac.caltech.edu in the data reduction. We measured the gas evolution (HI mass), gas mass-to-luminosity ratio, and abundance of the elements such as the oxygen abundance for these galaxies. Our results show a big discrepancy between the behavior of LSBGs at low and high luminosity ranges. We find that the LSBGs have higher HI masses than other samples of BCGs. BCGs are forced to stem from LSBGs or from dlrs according to their gas to light ratio vs total luminosity value galaxies, Low Surface Brightness Galaxies, galaxies evolution, gas rich galaxies Science Q In Ibn Al-Haitham Journal for Pure and Applied Sciences University of Baghdad, 2019 26(2017), 2 (DE-627)756825806 (DE-600)2727526-7 25213407 nnns volume:26 year:2017 number:2 https://doaj.org/article/ea66cc69b4b14ae8892556fe11c72a83 kostenfrei https://jih.uobaghdad.edu.iq/index.php/j/article/view/484 kostenfrei https://doaj.org/toc/1609-4042 Journal toc kostenfrei https://doaj.org/toc/2521-3407 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 26 2017 2
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author	Layali Y. Al-Mashhadani
spellingShingle	Layali Y. Al-Mashhadani misc galaxies, Low Surface Brightness Galaxies, galaxies evolution, gas rich galaxies misc Science misc Q Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band)
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topic_title	Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band) galaxies, Low Surface Brightness Galaxies, galaxies evolution, gas rich galaxies
topic	misc galaxies, Low Surface Brightness Galaxies, galaxies evolution, gas rich galaxies misc Science misc Q
topic_unstemmed	misc galaxies, Low Surface Brightness Galaxies, galaxies evolution, gas rich galaxies misc Science misc Q
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title	Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band)
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title_full	Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band)
author_sort	Layali Y. Al-Mashhadani
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title_sort	comments on properties of gas rich dwarfs galaxies in the range of radio frequencies (b-band)
title_auth	Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band)
abstract	In this project we analyze data of a large sample of gas rich dwarfs galaxies including; Low Surface Brightness Galaxies (LSBGs), Blue Compact Galaxies (BCGs), and dwarfs Irregulars (dIr). We then study the difference between properties of these galaxies in the range of radio frequencies (B-band). The data are available in HIPASS catalogue and McGaughâ€™s Data Page. We depended also NASA/IPACExtragalactic Databes web site http://ned.ipac.caltech.edu in the data reduction. We measured the gas evolution (HI mass), gas mass-to-luminosity ratio, and abundance of the elements such as the oxygen abundance for these galaxies. Our results show a big discrepancy between the behavior of LSBGs at low and high luminosity ranges. We find that the LSBGs have higher HI masses than other samples of BCGs. BCGs are forced to stem from LSBGs or from dlrs according to their gas to light ratio vs total luminosity value
abstractGer	In this project we analyze data of a large sample of gas rich dwarfs galaxies including; Low Surface Brightness Galaxies (LSBGs), Blue Compact Galaxies (BCGs), and dwarfs Irregulars (dIr). We then study the difference between properties of these galaxies in the range of radio frequencies (B-band). The data are available in HIPASS catalogue and McGaughâ€™s Data Page. We depended also NASA/IPACExtragalactic Databes web site http://ned.ipac.caltech.edu in the data reduction. We measured the gas evolution (HI mass), gas mass-to-luminosity ratio, and abundance of the elements such as the oxygen abundance for these galaxies. Our results show a big discrepancy between the behavior of LSBGs at low and high luminosity ranges. We find that the LSBGs have higher HI masses than other samples of BCGs. BCGs are forced to stem from LSBGs or from dlrs according to their gas to light ratio vs total luminosity value
abstract_unstemmed	In this project we analyze data of a large sample of gas rich dwarfs galaxies including; Low Surface Brightness Galaxies (LSBGs), Blue Compact Galaxies (BCGs), and dwarfs Irregulars (dIr). We then study the difference between properties of these galaxies in the range of radio frequencies (B-band). The data are available in HIPASS catalogue and McGaughâ€™s Data Page. We depended also NASA/IPACExtragalactic Databes web site http://ned.ipac.caltech.edu in the data reduction. We measured the gas evolution (HI mass), gas mass-to-luminosity ratio, and abundance of the elements such as the oxygen abundance for these galaxies. Our results show a big discrepancy between the behavior of LSBGs at low and high luminosity ranges. We find that the LSBGs have higher HI masses than other samples of BCGs. BCGs are forced to stem from LSBGs or from dlrs according to their gas to light ratio vs total luminosity value
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title_short	Comments on Properties of Gas Rich Dwarfs Galaxies in the Range of Radio Frequencies (B-Band)
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