SiO Maser Survey of IRAS Sources in the Inner Galactic Disk

Deguchi Shuji; Fujii Takahiro; Glass Ian S.; Imai Hiroshi; Ita Yoshifusa; Izumiura Hideyuki; Kameya Osamu; Miyazaki Atsushi; Nakada Yoshikazu; Nakashima Jun-ichi

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SiO Maser Survey of IRAS Sources in the Inner Galactic Disk

机译：内银河盘中IRAS源的SiO Maser调查

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Wesurveyed401color-selectedIRASsourcesinthegalacticdiskintheSiO$$J=1hbox{--}0,v=1$$and2maserlinesat43a€‰GHz,resultingin254(239new)detections.Theobservedsourcesliemostlyinastripoftheinnergalacticdiskwithboundaries$$-10^{circ}l40^{circ}$$and$$vertbvert3^{circ}$$.Thissurveyprovidesradialvelocitiesofinner-diskstarsforwhichopticalmeasurementscannotbemadeduetointerstellarextinction.TheSiO$$lhbox{--}v$$diagraminthearea$$-10^{circ}l40^{circ}$$exhibitsfewerobjectscoincidentwiththemolecularringfeaturethandoestheOH1612a€‰MHzsource$$lhbox{--}v$$map,indicatingaslightdifferenceofstellartypebetweenSiOandOHemittingstars.AfteridentifyingalloftheSiOdetectedsourcesinthe2MASSnear-infraredcatalog,wecomputedtheirluminositydistancesbasedontheinfraredfluxes.Wethenmappedtheseobjectsontothefirstquadrantofthegalacticplane.CombiningthedistanceswiththeSiOradialvelocities,weobtainedapatternspeedforSiOmasersources,$$Omega_{mathrm{P}}=21(pm13),mathrm{km},mathrm{s}^{-1},mathrm{kpc}^{-1}$$,betweenthedistances1and5.5a€‰kpc,withouttheuseofanydynamicalmodels.Theincreaseofthepatternspeedtowardthegalacticcenter(upto$$60,mathrm{km},mathrm{s}^{-1},mathrm{kpc}^{-1}$$betweenthedistances,5.5and7a€‰kpc)suggeststhepresenceoftwopatternspeedsintheGalaxy.

机译：我们对SiO $$ J = 1hbox {-} 0，v = 1 $$和2个母线在43aGHz的银河盘中的401种颜色选定的IRAS源进行了检测，结果发现了254（239new）次。所观察到的源几乎是带星界的银河星盘的条带$$-10 ^ {circ} $$$ {40 ^ SiO $$ lhbox {-} v $$ diagraminthearea $ -10 ^ {circtltllllthewithweakthefeaturingwithfescopefefethingfeaturethofthescopeofthescopefeaturingwithfeaturingfeaturingwithfeaturingfeaturingwithfeaturingfeaturingwithfeaturingfeaturingthescoefeatures.jpg。$$ vertbvert 3 ^ {circ} $$。此调查提供了由于盘内消光而无法进行光学测量的内盘星的径向速度。 ‰MHzsource $$ lhbox { - }伏$$地图，indicatingaslightdifferenceofstellartypebetweenSiOandOHemittingstars.AfteridentifyingalloftheSiOdetectedsourcesinthe2MASSnear-infraredcatalog，wecomputedtheirluminositydistancesbasedontheinfraredfluxes.Wethenmappedtheseobjectsontothefirstquadrantofthegalacticplane.CombiningthedistanceswiththeSiOradialvelocities，weobtainedapatternspeedforSiOmasersources，$$ Omega_ {mathrm {P}} = 21（PM13），mathrm {公里}，{mathrm s} ^ {-1}，mathrm {kpc} ^ {-1} $$，介于则建议在不使用任何动态模型的情况下先增加1和5.5kpc的速度。建议将模式速度向银河中心移动（最高$ 60，mathrm {km}，mathrm {s} ^ {-1}，mathrm {kpc} ^ {-1} $在距离之间，$ 5.5和7a€kpc的速度建议这两个值。。

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《PASJ: Publications of the Astronomical Society of Japan》 |2004年第5期|共页
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Deguchi Shuji; Fujii Takahiro; Glass Ian S.; Imai Hiroshi; Ita Yoshifusa; Izumiura Hideyuki; Kameya Osamu; Miyazaki Atsushi; Nakada Yoshikazu; Nakashima Jun-ichi;
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1. SiO maser survey of the galactic disk IRAS sources. II. vertical bar l vertical bar <= 3 degrees and vertical bar b vertical bar <= 3 degrees, the Galactic center area [J] . Deguchi S., Izumiura H., Kameya O., The Astrophysical Journal. Supplement Series . 2000,第2期

机译：SiO Maser对银河磁盘IRAS来源的调查。 II。垂直条L垂直条<= 3度和垂直条B垂直条<= 3度，银河系中心区域
2. SiO maser survey of the galactic disk IRAS sources. I. 15 deg < l < 25 deg, near end of the galactic bar [J] . Hideyuki Izumiura, Shuji Deguchi, Takahiro Fujii, The Astrophysical Journal. Supplement Series . 1999,第1期

机译：SiO maser对银河盘IRAS源的调查。 I. 15度
3. SiO maser survey of IRAS sources in the inner galactic disk [J] . Deguchi S, Fujii T, Glass IS, PASJ: Publications of the Astronomical Society of Japan . 2004,第5期

机译：内银河盘中IRAS源的SiO maser调查
4. SiO Maser Survey of IRAS Bulge Sources [C] . HIDEYUKI IZUMIURA, I. YAMAMURA, S. DEGUCHI, IAA-IAC-University of Pisa Workshop . 1995

机译：SIO MASER对IRAS凸起来源调查
5. Astrophysical maser radiation from Keplerian disks near active galactic nuclei. [D] . Wallin, Bradley Karl. 1998

机译：来自活跃银河原子核附近的开普勒圆盘的天体物理激射辐射。
6. High-resolution observations of IRAS 08544–4431: Detection of a disk orbiting a post-AGB star and of a slow disk wind [O] . V. Bujarrabal, A. Castro-Carrizo, H. Van Winckel, -1

机译：IRAS 08544–4431的高分辨率观测：检测到绕AGB后恒星运行的磁盘和慢速的磁盘风
7. SiO maser survey of the Galactic disk IRAS sources. II. l ≤ 3° and b ≤ 3°, the Galactic center area [O] . Kameya O, Nakada Y, Nakashima JI, 2000

机译：关于银河系IRas源的siO脉泽测量。 II。 L ≤3°和 b ≤3°，银河系中心区
8. Papers Presented at the Conference on 'Astrophysical Masers'. Held in Washington, DC. on March 9-11, 1992. Space VLBI and the Masers. A VLBI Survey of Interstellar Broadening of Galactic OH Masers. Properties of OH/IR Stars in the Galactic Centre. [R] . Booth, R. S., Hansen, J., Dennison, B., 1992

机译：论文发表在“天体物理学杂志”上。在华盛顿特区举行。 1992年3月9日至11日。太空VLBI和masers。星际拓展银河系OH masers的VLBI调查。银河系中心OH / IR星的特性。

SiO Maser Survey of IRAS Sources in the Inner Galactic Disk

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