SiO Maser Observations toward Orion-KL with VERA

By Mi Kyoung Kim, T. Hirota, M. Honma, H. Kobayashi, T. Bushimata, Y. Choi, H. Imai, K. Iwadate, T. Jike, S. Kameno and 22 more. 2008

142 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/cd67a39c0312bea937ab1a91a9d61ff35a1107eb

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Citations in the corpus

THE GOULD’S BELT DISTANCES SURVEY (GOBELINS). II. DISTANCES AND STRUCTURE TOWARD THE ORION MOLECULAR CLOUDS (2016, methodology): “Sandstrom et al. (2007, hereafter S07) also observed GMR A and obtained a somewhat closer distance of - +389 21 24 pc. Hirota et al. (2007) and Kim et al. (2008) observed H2O and SiO masers to obtain a distance of 437±19 pc and 418±6 pc respectively in the Orion BN/KL region.”
TRIGONOMETRIC PARALLAXES OF HIGH MASS STAR FORMING REGIONS: THE STRUCTURE AND KINEMATICS OF THE MILKY WAY (2014, unknown): “…39:Niinuma et al. (2011), 40:Reid et al. (2009a), 41:Shiozaki et al. (2011), 42:Honma et al. (2007), 43:Sandstrom et al. (2007),4 4:Menten et al. (2007), 45:Kim et al. (2008), 46:Choi et al. (2008), 47:Zhang et al. (2012a). most straightforwardly, looking at a plan view of the Milky Way (see Fig.”
AN OPTICAL SPECTROSCOPIC STUDY OF T TAURI STARS. I. PHOTOSPHERIC PROPERTIES (2014, background): “…pc for stars near the Lynds 1495 complex in Taurus (Torres et al. 2012), 147 pc for stars near T Tau (Loinard et al. 2007), 161 pc for the stars near the HP Tau complex in Taurus (Torres et al. 2009), 140 pc for all other Taurus objects, and 416 pc for Orion (Menten et al. 2007; Kim et al. 2008).”
The Bar and Spiral Structure Legacy (BeSSeL) Survey: Mapping the Milky Way with VLBI Astrometry† (2011, unknown): “The most accurate measurements of 414 ± 7 pc (Menten et al. 2007, VLBA, 4 radio stars) and 418 ± 6 pc (Kim et al. 2008, VERA, SiO maser) also agree with each other and with the modeling of the orbit of the binary Θ1 Ori C from near-infrared interferometry (Kraus et al. 2007, 434±12 pc).”
ON THE NATURE OF THE LOCAL SPIRAL ARM OF THE MILKY WAY (2013, background): “…et al. (2007) and Kim et al. (2008) with equal accuracy, while the proper motions come fromMenten et al. (2007), because Hirota et al. (2007) and Kim et al. (2008) only use one spot to estimate these values. eThe parallax of VY CMa is unweighted average value of the independent results from…”
Accretion disks in luminous young stellar objects (2015, unknown): “…Palau et al. (2013); 15: Gueth et al. (2001); 16: Palau et al. (2010); 17: Fuente et al. (2001); 18: Fuente et al. (2005); 19: Fontani et al. (2004a); 20: Kim et al. (2008); 21: Crimier et al. (2009); 22: López-Sepulcre et al. (2013); 23: Launhardt & Henning (1997); 24: Felli et al. (2004); 25:…”
Fundamental Parameters of the Milky Way Galaxy Based on VLBI Astrometry (2012, unknown): “…(6) Dzib et al. 2010, (7) Hachisuka et al. 2009, (8) Hirota et al. 2008a, (9) Hirota et al. 2008b, (10) Hirota et al. 2011, (11) Honma et al. 2007, (12) Imai et al. 2007, (13) Kim et al. 2008, (14) Loinard et al. 2007, (15) Loinard et al. 2008, (16) Moellenbrock et al. 2009, (17) Moscadelli…”
Microarcsecond Radio Astrometry (2013, methodology): “Recently, two very accurate parallaxes have been published: Menten et al. (2007) used the VLBA and observed continuum emission from three YSOs and determined a distance of 414±7 pc; Kim et al. (2008) using VERA and observing SiO masers estimated a distance of 418±6 pc.”
THE HERSCHEL ORION PROTOSTAR SURVEY: SPECTRAL ENERGY DISTRIBUTIONS AND FITS USING A GRID OF PROTOSTELLAR MODELS (2016, background): “This is the largest sample of protostars studied in a single, nearby starforming region (distance of 420 pc; Menten et al. 2007; Kim et al. 2008) and therefore significant for advancing our understanding of protostellar structure and evolution.”