The association of IL1α and IL1β polymorphisms with susceptibility to systemic lupus erythematosus: A meta-analysis

Wang, Bin; Zhu, Ji-Min; Fan, Yin‐Guang; Feng, Chen-Chen; Chen, Gui-Mei; Chen, Hong; Pan, Hai‐Feng; Ye, Dong-Qing

doi:10.1016/j.gene.2013.05.059

Cited by 22 publications

(31 citation statements)

References 36 publications

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“…The velocities and widths of the two distinctive kinematic components of the methanol line map are generally consistent with their first detection in the earliest methanol observations by Menten et al (1986) and Wilson et al (1989), of a single transition of the 23 GHz 10-9 A − band. The present results are also consistent with HIFI observations of the ΔJ=0, = - -K 4 3 and =  K 7 6 v t =0 Q-branch transitions at 524 and 1061 GHz by Wang et al (2011), at a fixed position centered on the Hot Core. These distinct components were demonstrated by Wang et al to probe gas at different temperatures.…”

Section: Ch 3 Oh K=5 ↔ 4 (E)supporting

confidence: 91%

“…At the higher angular resolution of the interferometric data, ;3 0, emission peaks are resolved around five narrow LSR velocity ranges centered at 3, 5, 8, 11, and >12 km s −1 . Feng et al quote that these lines are all broad, ∼5-7 km s −1 , apparently lacking the additional narrow <3 km s −1 component observed by Menten et al (1986), Wilson et al (1989), Wang et al (2011), and in our data.…”

Section: Ch 3 Oh K=5 ↔ 4 (E)contrasting

confidence: 50%

“…Concerning spatial distribution, Wang et al (2011) associated the narrow component with signatures of the Compact Ridge, which is usually approximated as a spherical clump of molecular gas 5″-10″ in diameter (an idea put forth by Blake et al 1987), and externally heated to produce the relatively low velocity widths. Menten et al (1986Menten et al ( , 1988 had previously identified the narrow component with a larger region ≈25″ in size, centered 5″-10″ south of the Hot Core where the broad emission component peaks.…”

Section: Ch 3 Oh K=5 ↔ 4 (E)mentioning

confidence: 99%

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HERSCHEL/HIFI SPECTRAL MAPPING OF C⁺, CH⁺, AND CH IN ORION BN/KL: THE PREVAILING ROLE OF ULTRAVIOLET IRRADIATION IN CH⁺ FORMATION

Morris

Gupta

Nagy

et al. 2016

ApJ

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The CH + ion is a key species in the initial steps of interstellar carbon chemistry. Its formation in diverse environments where it is observed is not well understood, however, because the main production pathway is so endothermic (4280 K) that it is unlikely to proceed at the typical temperatures of molecular clouds. We investigate the formation of this highly reactive molecule with the first velocity-resolved spectral mapping of the CH + J= 1−0, 2−1 rotational transitions, three sets of CH Λ-doubled triplet lines, 12 C + and 13 C + P P , and CH is indicated to arise in the diluted gas, outside the explosive, dense BN/KL outflow. Our models show that UV irradiation provides favorable conditions for steady-state production of CH + in this environment. Surprisingly, no spatial or kinematic correspondences of the observed species are found with H 2 S(1) emission tracing shocked gas in the outflow. We propose that C + is being consumed by rapid production of CO to explain the lack of both C + and CH + in the outflow. Hence, in star-forming environments containing sources of shocks and strong UV radiation, a description of the conditions leading to CH + formation and excitation is incomplete without including the important-possibly dominant-role of UV irradiation.

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Section: Ch 3 Oh K=5 ↔ 4 (E)supporting

confidence: 91%

Section: Ch 3 Oh K=5 ↔ 4 (E)contrasting

confidence: 50%

Section: Ch 3 Oh K=5 ↔ 4 (E)mentioning

confidence: 99%

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HERSCHEL/HIFI SPECTRAL MAPPING OF C⁺, CH⁺, AND CH IN ORION BN/KL: THE PREVAILING ROLE OF ULTRAVIOLET IRRADIATION IN CH⁺ FORMATION

Morris

Gupta

Nagy

et al. 2016

ApJ

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“…[1][2][3][4][5][6][7][8][9][10][11] The range of relevant temperatures is very broad, from 5 K up to 2500 K, and the role of scattering partner (quencher) is played by the interstellar background gasses, mostly He and H 2 , but also by H 2 O in cometary comas. Usually, calculations of inelastic cross sections 12 are carried out using quantum scattering codes such as MOLSCAT.…”

Section: Introductionmentioning

confidence: 99%

Mixed quantum/classical theory of rotationally and vibrationally inelastic scattering in space-fixed and body-fixed reference frames

Семенов

Babikov

2013

The Journal of Chemical Physics

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We formulated the mixed quantum/classical theory for rotationally and vibrationally inelastic scattering process in the diatomic molecule + atom system. Two versions of theory are presented, first in the space-fixed and second in the body-fixed reference frame. First version is easy to derive and the resultant equations of motion are transparent, but the state-to-state transition matrix is complexvalued and dense. Such calculations may be computationally demanding for heavier molecules and/or higher temperatures, when the number of accessible channels becomes large. In contrast, the second version of theory requires some tedious derivations and the final equations of motion are rather complicated (not particularly intuitive). However, the state-to-state transitions are driven by realvalued sparse matrixes of much smaller size. Thus, this formulation is the method of choice from the computational point of view, while the space-fixed formulation can serve as a test of the bodyfixed equations of motion, and the code. Rigorous numerical tests were carried out for a model system to ensure that all equations, matrixes, and computer codes in both formulations are correct.

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“…Herschel surveys toward different sources revealed many spectral features that we currently cannot identify (e.g. Wang et al 2011). However, no unidentified lines were found in our spectra.…”

Section: Detections and Line Profilesmentioning

confidence: 54%

The HIFI spectral survey of AFGL 2591 (CHESS)

Kaźmierczak-Barthel

Tak

Helmich

et al. 2014

A&A

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Aims. This paper presents the richness of submillimeter spectral features in the high-mass star forming region AFGL 2591. Methods. As part of the Chemical Herschel Survey of Star Forming Regions (CHESS) key programme, AFGL 2591 was observed by the Herschel (HIFI) instrument. The spectral survey covered a frequency range from 480 to 1240 GHz as well as single lines from 1267 to 1901 GHz (i.e. CO, HCl, NH 3 , OH, and [CII]). Rotational and population diagram methods were used to calculate column densities, excitation temperatures, and the emission extents of the observed molecules associated with AFGL 2591. The analysis was supplemented with several lines from ground-based JCMT spectra. Results. From the HIFI spectral survey analysis a total of 32 species were identified (including isotopologues). Although the lines are mostly quite weak ( T mb dV∼ few K km s −1 ), 268 emission and 16 absorption lines were found (excluding blends). Molecular column densities range from 6 × 10 11 to 1 × 10 19 cm −2 and excitation temperatures from 19 to 175 K. Cold (e.g. HCN, H 2 S, and NH 3 with temperatures below 70 K) and warm species (e.g. CH 3 OH, SO 2 ) in the protostellar envelope can be distinguished.

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The association of IL1α and IL1β polymorphisms with susceptibility to systemic lupus erythematosus: A meta-analysis

Cited by 22 publications

References 36 publications

HERSCHEL/HIFI SPECTRAL MAPPING OF C⁺, CH⁺, AND CH IN ORION BN/KL: THE PREVAILING ROLE OF ULTRAVIOLET IRRADIATION IN CH⁺ FORMATION

HERSCHEL/HIFI SPECTRAL MAPPING OF C⁺, CH⁺, AND CH IN ORION BN/KL: THE PREVAILING ROLE OF ULTRAVIOLET IRRADIATION IN CH⁺ FORMATION

Mixed quantum/classical theory of rotationally and vibrationally inelastic scattering in space-fixed and body-fixed reference frames

The HIFI spectral survey of AFGL 2591 (CHESS)

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The association of IL1α and IL1β polymorphisms with susceptibility to systemic lupus erythematosus: A meta-analysis

Cited by 22 publications

References 36 publications

HERSCHEL/HIFI SPECTRAL MAPPING OF C+, CH+, AND CH IN ORION BN/KL: THE PREVAILING ROLE OF ULTRAVIOLET IRRADIATION IN CH+ FORMATION

HERSCHEL/HIFI SPECTRAL MAPPING OF C+, CH+, AND CH IN ORION BN/KL: THE PREVAILING ROLE OF ULTRAVIOLET IRRADIATION IN CH+ FORMATION

Mixed quantum/classical theory of rotationally and vibrationally inelastic scattering in space-fixed and body-fixed reference frames

The HIFI spectral survey of AFGL 2591 (CHESS)

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Product

Resources

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HERSCHEL/HIFI SPECTRAL MAPPING OF C⁺, CH⁺, AND CH IN ORION BN/KL: THE PREVAILING ROLE OF ULTRAVIOLET IRRADIATION IN CH⁺ FORMATION

HERSCHEL/HIFI SPECTRAL MAPPING OF C⁺, CH⁺, AND CH IN ORION BN/KL: THE PREVAILING ROLE OF ULTRAVIOLET IRRADIATION IN CH⁺ FORMATION