Common Correlations between 60, 100, and 140$, {mu mathrm {m}}$ Intensities in the Galactic Plane and Magellanic Clouds

Hibi Yasunori; Shibai Hiroshi; Kawada Mitsunobu; Ootsubo Takafumi; Hirashita Hiroyuki

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Common Correlations between 60, 100, and 140$, {mu mathrm {m}}$ Intensities in the Galactic Plane and Magellanic Clouds

机译：银河平面和麦哲伦星云中60、100和140 $，{mu mathrm {m}} $强度之间的常见相关性

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Weinvestigatedthefar-infraredSEDoftheGalaxyandtheMagellanicCloudsbyusingtheCOBE(COsmicBackgroundExplorer)/DIRBE(DiffuseInfraRedBackgroundExperiment)ZSMA(Zodi-SubtractedMissionAverage)mapsatwavelengthsof60$$,{mumathrm{m}}$$,100$$,{mumathrm{m}}$$,and140$$,{mumathrm{m}}$$.Weanalyzedthreeregions:thegalacticplaneregionwiththegalacticlatitude$$vertbvert5^{circ}$$,theLargeMagellanicCloudregion,andtheSmallMagellanicCloudregion.Becausethedustopticaldepthismuchsmallerinthefar-infraredthaninthevisible,wecouldobservecumulativefar-infraredradiationfromregionswithvariousinterstellarradiationfieldinthelineofsight.Asaconsequenceofconsideringsuchaneffect,wefoundacommonfar-infraredcolorcorrelationbetweenthe140a€“100$$,{mumathrm{m}}$$and100a€“60$$,{mumathrm{m}}$$intensityratiosinallthreegalaxies.Althoughthiscolorcorrelationcannotbeexplainedbyanyexistingmodel,itfitsverywellthefar-infraredcolorofnearbystar-forminggalaxies.

机译：我们通过使用波长为60 $$，{$ math，{$ r的COBE（COSmicBackgroundExplorer）/ DIRBE（DiffuseInfraRedBackexperiment）ZSMA（Zodi-SubtractedMissionAverage）ZSMA映射图研究了银河和麦哲伦星云的远红外SED。 ... M}} $$ Weanalyzedthreeregions：CTI的思想CPLA是希腊谁NWI ththe认为CTI克劳迪娅纬度$$的vertbvert 5 ^ {保监会} $$，theLargeMagellanicCloudregion，andtheSmallMagellanicCloudregion.Becausethedustopticaldepthismuchsmallerinthefar-的NFRA到DTHA改变可见，wecouldobservecumulativefar-infraredradiationfromregionswithvariousinterstellarradiationfieldinthelineofsight.Asaconsequenceofconsideringsuchaneffect，wefoundacommonfar-的NFRA一个DCO一个RCO我们NBE TWE enthe140a€的RRE“100 $$，{mumathrm {S}} $$和100a€“ 60 $$，{mumathrm {m}} $$强度在所有三个星系中的比率。尽管任何现有的模型都无法解释这种颜色相关性，但它非常适合恒星形成星系附近的远红外颜色。

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《PASJ: Publications of the Astronomical Society of Japan》 |2006年第3期|共页
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Hibi Yasunori; Shibai Hiroshi; Kawada Mitsunobu; Ootsubo Takafumi; Hirashita Hiroyuki;
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1. Common correlations between 60, 100, and 140 mu m intensities in the galactic plane and Magellanic Clouds [J] . Hibi Y, Shibai H, Kawada M, PASJ: Publications of the Astronomical Society of Japan . 2006,第3期

机译：银河平面和麦哲伦星云中60、100和140μm强度之间的常见相关性
2. Marseille Observatory Hα Survey of the Southern Galactic Plane and Magellanic Clouds [J] . D. Russeil Publications of the Astronomical Society of Australia . 2013,第1期

机译：马赛天文台南银河平面和麦哲伦星云的Hα测量
3. THE MAGELLANIC QUASARS SURVEY. III. SPECTROSCOPIC CONFIRMATION OF 758 ACTIVE GALACTIC NUCLEI BEHIND THE MAGELLANIC CLOUDS [J] . Szymon Koz?owski19, Christopher A. Onken2, Christopher S. Kochanek34, The Astrophysical journal . 2013,第2期

机译：麦哲伦四方调查。三，麦哲伦星云下758颗活性银河核素的光谱确认
4. A CMOS Proximity Capacitance Image Sensor with $16mu mathrm{m}$ Pixel Pitch, 0.1aF Detection Accuracy and 60 Frames Per Second [C] . M. Yamamoto, R. Kuroda, M. Suzuki, IEEE International Electron Devices Meeting . 2018

机译：具有 $ 16 mu mathrm {m} $ 像素间距，0.1aF检测精度和每秒60帧的CMOS接近电容图像传感器
5. Fuel for the Star Formation Engine: Dense Molecular Cloud Clumps in the Northern Galactic Plane [D] . Zetterlund, Erika. 2018

机译：用于星形形成引擎的燃料：北永曲面的密集分子云团块
6. MAGELLANIC CLOUDS. XIII. COMPARISON OF MAGELLANIC AND GALACTIC ECLIPSING VARIABLES [O] . Henry Norris Russell 1954

机译：麦哲伦云。十三。麦哲伦和银河日食变种的比较
7. Common Correlations between 60, 100, and 140$, {mu mathrm {m}}$ Intensities in the Galactic Plane and Magellanic Clouds [O] . Yasunori Hibi, Hiroshi Shibai, Mitsunobu Kawada, 2006

机译：在银河飞机和Magellanic云中的60,100和140 $ ，{ mathrm {m}}的常见相关性

Common Correlations between 60, 100, and 140$, {mu mathrm {m}}$ Intensities in the Galactic Plane and Magellanic Clouds

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