1973
DOI: 10.1086/181346
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High-Resolution Maps of the Kleinmann-Low Nebula in Orion

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Cited by 60 publications
(35 citation statements)
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“…The LTE fit was performed using LINEDB and WEEDS sets of routines inside CLASS (Maret et al 2011). The line catalogues are the Cologne Database for Molecular Spectroscopy (CDMS, Müller et al 2001Müller et al , 2005 and the Jet Propulsion Laboratory (JPL) catalogue (Pickett et al 1998), with some complementary data provided by A. Belloche from the Belloche et al (2013, hereafter B13) work to identify vibrationally excited states of vinyl and ethyl cyanides which we do not discuss in this paper but which were needed since a number of these transitions are very strong, up to 30 K. Rieke et al (1973), Shuping et al (2004), mmxx from Feng et al (2015) and references therein. The yellow cross indicates the center of explosion from which the BN, I, and n sources (marked by yellow stars) are moving away (Gómez et al 2005 …”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…The LTE fit was performed using LINEDB and WEEDS sets of routines inside CLASS (Maret et al 2011). The line catalogues are the Cologne Database for Molecular Spectroscopy (CDMS, Müller et al 2001Müller et al , 2005 and the Jet Propulsion Laboratory (JPL) catalogue (Pickett et al 1998), with some complementary data provided by A. Belloche from the Belloche et al (2013, hereafter B13) work to identify vibrationally excited states of vinyl and ethyl cyanides which we do not discuss in this paper but which were needed since a number of these transitions are very strong, up to 30 K. Rieke et al (1973), Shuping et al (2004), mmxx from Feng et al (2015) and references therein. The yellow cross indicates the center of explosion from which the BN, I, and n sources (marked by yellow stars) are moving away (Gómez et al 2005 …”
Section: Discussionmentioning
confidence: 99%
“…The core is complex with several remarkable sources, the hot core (HC), the compact ridge (CR), the extended ridge (ER), the plateau, numerous methyl formate (MF) peaks (Favre et al 2011a), and other infrared/submillimeter peaks listed in many papers (e.g. Rieke et al 1973;Robberto et al 2005;Friedel & Weaver 2011), including three runaway objects: BN, I, and n (Gómez et al 2005;Rodríguez et al 2005Rodríguez et al , 2017. Among the studies aimed at identifying molecules in Orion, which is the reference source along with Sgr B2 in which to search for new species, many surveys have been conducted with single-dish telescopes from the ground (from some of the earliest works by Sutton et al 1985;Blake et al 1986, to recent observations with the IRAM-30 m, Tercero et al 2010Tercero et al , 2011Cernicharo et al 2016;etc.…”
Section: Introductionmentioning
confidence: 99%
“…In the infrared McCaughrean & Stau †er numbers are given ; we recover all stars from that survey except for a few close pairsÈMS-86 is a close companion to P-1889, MS-65 is a close companion to P-1891 (#1C Ori), and MS-75 and MS-77 appear as a single source in our images. Lonsdale (1982), , and Rieke et al (1973) cross-identiÐcations are made. Finally, D250 of the sources with K \ 14.5 mag in Table 1 are also listed as point sources by 2MASS.…”
Section: Properties Of Final Source L Istmentioning
confidence: 99%
“…Up to now the situation has been con fused by resolution effects in VLBI measurements. (Rieke et al 1973) has the richest H 2 0 spectrum in number of lines and in the strongest integrated emission. It dominates H 2 0 VLBI maps on baselines >600 km, such as Onsala-Bonn and Haystack-NRAO.…”
Section: 1mentioning
confidence: 99%
“…The new H 2 0 VLBI maps show that it has low velocity emission near 6-7 km s" 1 and high velocity emission at 68.6, and 70.5 km s" 1 . It is also located near the peak of The VLBI positions of the low-velocity H 2 0 features are shown as black dots , superimposed on the contours of 20 ym infrared radiation (Wynn-Williams and Becklin 1974;Rieke et al 1973). Shaded circles represent compact infrared objects.…”
Section: The Infrared Source Irc4mentioning
confidence: 99%