1,723,559 research outputs found
RX J0123.4-7321-the story continues: major circumstellar disc loss and recovery
No full textABSTRACT
RX J0123.4-7321 is a well-established Be star X-ray binary system in the Small Magellanic Cloud. Like many such systems, the variable X-ray emission is driven by the underlying behaviour of the mass donor Be star. Previous work has shown that the optical and X-ray were characterized by regular outbursts at the proposed binary period of 119 d. However, around 2008 February the optical behaviour changed substantially, with the previously regular optical outbursts ending. Reported here are new optical (OGLE) and X-ray (Swift) observations covering the period after 2008 that suggest an almost total circumstellar disc loss followed by a gradual recovery. This indicates the probable transition of a Be star to a B star, and back again. However, at the time of the most recent OGLE data (2020 March) the characteristic periodic outbursts had yet to return to their early state, indicating that the disc still had some re-building yet to complete
RX J0123.4-7321-the story continues: major circumstellar disc loss and recovery
No full textABSTRACT
RX J0123.4-7321 is a well-established Be star X-ray binary system in the Small Magellanic Cloud. Like many such systems, the variable X-ray emission is driven by the underlying behaviour of the mass donor Be star. Previous work has shown that the optical and X-ray were characterized by regular outbursts at the proposed binary period of 119 d. However, around 2008 February the optical behaviour changed substantially, with the previously regular optical outbursts ending. Reported here are new optical (OGLE) and X-ray (Swift) observations covering the period after 2008 that suggest an almost total circumstellar disc loss followed by a gradual recovery. This indicates the probable transition of a Be star to a B star, and back again. However, at the time of the most recent OGLE data (2020 March) the characteristic periodic outbursts had yet to return to their early state, indicating that the disc still had some re-building yet to complete
Evidence for a large stellar bar in the Low Surface Brightness galaxy UGC 7321
No full textLate-type spiral galaxies are thought to be the dynamically simplest
type of disk galaxy and our understanding of their properties plays
a key role in galaxy formation and evolution scenarios.
The low surface brightness (LSB) galaxy UGC 7321, a nearby,
isolated, “superthin” edge-on galaxy, is an ideal object to study these
purely disk-dominated bulge-less galaxies.
Although late type spirals are believed to exhibit the simplest
possible structure, even prior observations showed deviations
from a pure single component exponential disk in the case of UGC 7321.
We present for the first time photometric evidence for peanut-shaped
outer isophotes from a deep optical (R-band) image of UGC 7321.
Observations and dynamical modeling suggest that boxy/peanut-shaped
(b/p) bulges in general form through the buckling instability in bars
of the parent galaxy disks.
Together with recent HI observations supporting the presence of a
stellar bar in UGC 7321, this could be the earliest known case
of the buckling process during the evolutionary life of a LSB galaxy,
whereby material in the disk-bar has started to be pumped up above
the disk, but a genuine bulge has not yet formed
Going Beyond Counting First Authors in Author Co-citation Analysis
Get PDFThe present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
Variations on the Author
Get PDF“Variations on the Author” discusses two of Eduardo Coutinho’s recent films (Um Dia na Vida, from 2010, and Últimas Conversas, posthumously released in 2015) and their contribution to the general question of documentary authorship. The director’s filmography is characterized by a consistent yet self-effacing form of authorial self-inscription: Coutinho often features as an interviewer that rather than express opinions propels discourses; an interviewer that is good at listening. This mode of self-inscription characterizes him as an author who is not expressive but who is nonetheless markedly present on the screen. In Um Dia na Vida, however, Coutinho is completely absent form the image, while Últimas Conversas, on the contrary, includes a confessional prologue that moves the director from the margins to the center of his films. This article examines the ways in which these works stand out in the filmography of a director who offers new insights into the notion of cinematic authorship
Appropriate Similarity Measures for Author Cocitation Analysis
Get PDFWe provide a number of new insights into the methodological discussion about author cocitation analysis. We first argue that the use of the Pearson correlation for measuring the similarity between authors’ cocitation profiles is not very satisfactory. We then discuss what kind of similarity measures may be used as an alternative to the Pearson correlation. We consider three similarity measures in particular. One is the well-known cosine. The other two similarity measures have not been used before in the bibliometric literature. Finally, we show by means of an example that our findings have a high practical relevance.information science;Pearson correlation;cosine;similarity measure;author cocitation analysis
Draft genomes of Nautella italica CECT 7645T and CECT 7321: two roseobacters with potential pathogenic and biotechnological traits
No full textNautella italica is a member of the family Rhodobacteraceae described in 2009. Strain LMG 24365(T) (=CECT 7645(T), =DSM 26436(T), =CCUG 55857(T)) was isolated from a marine electroactive biofilm growing in a stainless steel cathode exposed to natural water in Genoa, Italy. Strain AD 41 (=CECT 7321) was isolated from water surrounding cultivated gilthead seabream larvae in Cádiz, Spain. The genomes of strains CECT 7645(T) and CECT 7321 were sequenced, assembled, annotated and compared. Here we describe the most relevant findings: biofilm formation, quorum sensing, resistance to multiple drugs, heavy metals and oxidative stress, cytotoxins, and poly-β-hydroxybutyrate (PHB) production genes. These genomes were also compared to current available genomes in NCBI Genome Database from members of the genus Nautella, Nautella sp. R11 and Nautella sp. ECSMB14104. The comparison showed a higher similarity between strains CECT 7645(T) and R11 compared to strain CECT 7321 and strain ECSMB14104. The genome similarity indexes allowed confirming and assigning strains CECT 7321, R11 and ECSMB14104 to the species N. italica
High Latitude HI in the Low Surface Brightness Galaxy UGC 7321
No full textFrom the analysis of sensitive H I 21 cm line observations, we find evidence for vertically extended H I emission (\z\ less than or similar to 2.4 kpc) in the edge-on, low surface brightness spiral galaxy UGC 7321. Three-dimensional modeling suggests that the H I disk of UGC 7321 is both warped and flared, but that neither effect can fully reproduce the spatial distribution and kinematics of the highest z-height gas. We are able to model the high-latitude emission as an additional H I component in the form of a "thick disk'' or "halo'' with a FWHM of similar to3.3 kpc. We find tentative evidence that the vertically extended gas declines in rotational velocity as a function of z, although we are unable to completely rule out models with constant V(z). In spite of the low star formation rate of UGC 7321, energy from supernovae may be sufficient to sustain this high-latitude gas. However, alternative origins for this material, such as slow, sustained infall, cannot yet be excluded.</p
Dispelling the Myths Behind First-author Citation Counts
Get PDFWe conducted a full-scale evaluative citation analysis study of scholars in the XML research field to explore just how different from each other author rankings resulting from different citation counting methods actually are, and to demonstrate the capability of emerging data and tools on the Web in supporting more realistic citation counting methods. Our results contest some common arguments for the continued
use of first-author citation counts in the evaluation of scholars, such as high correlations between author rankings by first-author citation counts and other citation
counting methods, and high costs of using more realistic citation counting methods that are not well-supported by the ISI databases. It is argued that increasingly available digital full text research papers make it possible for citation analysis studies to go beyond what the ISI databases have directly supported and to employ more
sophisticated methods
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