Synthesis and electrochemical performances of Mn x Co y Ni z CO3

Li, Qing; Hu, Yanling; Li, Lin; Feng, Chuanqi

doi:10.1007/s10854-015-3942-y

Cited by 40 publications

(61 citation statements)

References 35 publications

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“…This set includes both those objects that are classically considered to be "confirmed members" (e.g., Kenyon & Hartmann 1995;Luhman et al 2010;Rebull et al 2010), and those that were suggested as candidates but are not typically included in the widely used Taurus census papers (Wichmann et al 1996;Li & Hu 1998). We tabulate the full list of objects in Table 1 and plot their equatorial coordinate positions in Figure 1.…”

Section: Sample Constructionmentioning

confidence: 99%

“…We therefore consider the candidate Taurus members reported by Wichmann et al (1996), which were selected from a compilation of optical counterparts of X-ray sources from the ROSAT All-Sky Survey (Neuhauser et al 1995a), as well as 12 candidate Taurus members reported in a wider ROSAT survey by Li & Hu (1998) Neuhauser et al (1995b), and instead defer an even wider search until the population within our existing search area is determined more robustly. We also include 2 sources of uncertain membership reported by Scelsi et al (2008) as part of the XEST survey using XMM/Newton.…”

Section: Sample Constructionmentioning

confidence: 99%

“…High-resolution spectroscopic observations for 35 candidates from the surveys of Slesnick et al (2006b) and Li & Hu (1998) were previously obtained with Keck/HIRES on 2006 December 12 and 13 (PIs Carpenter and Slesnick). These observations are particularly useful in casting light on the nature of objects east of a = 5 h that Slesnick et al (2006b) suggested might be a distributed population of intermediate-age objects.…”

Section: Keck/hires High-resolution Optical Spectroscopymentioning

confidence: 99%

“…Of the confirmed or likely Taurus members, 81 sources (37%) have been largely omitted from the canonical Taurus census (e.g., Esplin et al 2014). Most of these missing sources are G-K stars drawn from the ROSAT-based surveys of Wichmann et al (1996) and Li & Hu (1998), suggesting that a substantial reservoir of unrecognized lower-mass members remains to be identified. However, we note that these new Taurus members are still the minority of all ROSAT-selected stars.…”

Section: An Updated Census Of Taurus-aurigamentioning

confidence: 99%

“…However, many 1 candidates have also been identified at larger distances from the classically accepted concentrations of young stars, leading to ongoing suggestions of a distributed (older) population (e.g., Wichmann et al 1996;Li & Hu 1998;Slesnick et al 2006b;Gómez de Castro et al 2015) where disks have largely already dispersed. Many of these claims have been subsequently considered and taken as evidence of contamination by interloper field stars (Briceno et al 1997), and the distributed candidates do not appear in most of the canonical target lists used for studies of Taurus (e.g., Kenyon & Hartmann 1995;Kenyon et al 2008;Luhman et al 2010).…”

Section: Introductionmentioning

confidence: 99%

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The Greater Taurus–Auriga Ecosystem. I. There is a Distributed Older Population

Kraus

Herczeg

Rizzuto

et al. 2017

ApJ

158

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The census of Taurus-Auriga has been assembled over seven decades and inherited the biases and incompleteness of the input studies. The unusual shape of its inferred initial mass function (IMF) and the existence of isolated diskbearing stars suggest that additional (likely disk-free) members remain to be discovered. We therefore have begun a global reassessment of the census of Taurus-Auriga that exploits new data and better definitions of youth and kinematic membership. As a first step, we reconsider the membership of all disk-free candidate members from the literature with spectral type F0, a < < 3 50 5 40 h m h m , and d  < <  14 34 . We combine data from the literature with Keck/HIRES and UH88/SNIFS spectra to test the membership of these candidates using the positions in the Hertzsprung-Russel diagram, proper motions, radial velocities, Hα, lithium, and surface gravity. We find 218 confirmed or likely Taurus members, 160 confirmed or likely interlopers, and only 18 that lack sufficient evidence to draw firm conclusions. A significant fraction of these stars (81/218 = 37%) are not included in the most recent canonical member lists. There are few additional members to the immediate vicinity of the molecular clouds, preserving the IMFs that have been deemed anomalous in past work. Many of the likely Taurus members are instead distributed broadly across the search area. When combined with the known disk hosts, our updated census reveals two regimes: a high-density population with a high disk fraction (indicative of youth) that broadly traces the molecular clouds, and a low-density population with low disk fraction (hence likely older) that most likely represents previous generations of star formation.

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Section: Sample Constructionmentioning

confidence: 99%

Section: Sample Constructionmentioning

confidence: 99%

Section: Keck/hires High-resolution Optical Spectroscopymentioning

confidence: 99%

Section: An Updated Census Of Taurus-aurigamentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

See 3 more Smart Citations

The Greater Taurus–Auriga Ecosystem. I. There is a Distributed Older Population

Kraus

Herczeg

Rizzuto

et al. 2017

ApJ

158

View full text Add to dashboard Cite

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Grain Morphology and Mechanical Properties Tailoring of Inconel 625 Alloy Fabricated by Laser Powder Bed Fusion

Zhou,

Peng,

et al. 2024

Adv Eng Mater

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The controlling strategies of grain morphology and mechanical properties of Inconel 625 alloy by laser powder bed fusion were investigated, and beyond that, the effects of phase composition, grain morphology and crystallographic texture on mechanical properties were also studied. The phase evolution was insensitive to the scanning strategies and all of the samples were composed of γ‐Ni phase. The (001) texture orientation tended to increase with the scanning rotation angle and the sample IV fabricated by scanning strategies of 90° shows the highest (001) texture. Different grain morphologies can be tailored by controlling the direction of heat flow between continuous layers via changing scanning strategies. The proportion of large elongated columnar crystals gradually decreases while the proportion of the equiaxed grains gradually increases as the scanning strategies change from 0°→90→ 67°→45°. The rotation angle increases from 0° to 45°, the ultimate tensile strength and yield strength increase from 1267±12MPa to 1304±5MPa and 760±10MPa to 801±5MPa, respectively, which is attributed to the different stress states presented in the columnar crystals and the equiaxed crystals.This article is protected by copyright. All rights reserved.

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