[PDF] Top 20 Giant molecular filaments in the Milky Way II. The fourth Galactic quadrant

... “The Milky Way System” and the International Max-Planck Research School (IMPRS) at Heidelberg ...their Galactic model and also for very useful discussions that helped to improve the ... See full document

... Most filaments have some association with – at most – a low level of star ...the Galactic context using a model of the Milky Way’s kine- matic ...first quadrant due to our orientation with ... See full document

... Milky Way. Furthermore, we can study the H i absorption spectra and molecular emission spectra of the Galactic point sources to estimate their distance and overcome the near-far distance ... See full document

... Observations of physical binary systems can lead to useful information about the relative luminosities of two stars at the same distance. The absolute magnitudes of many B type stars can thus be inferred from the ... See full document

... the Galactic bulge. The sample consists of 650 K giant stars spectra, from 3 fields along the Bulge minor axis ( b = − 4, − 6, − 12) and another field at ( l , b ) = ( − 5, − 4), obtained with the ... See full document

... between Galactic archaeology and cosmology, however, the difficulty in obtaining proper motions for all of the satellites makes it difficult to develop accurate ... See full document

... the Milky Way foreground stars by using photometric filters in the color-magnitude space and com- paring the integrated signal-to-noise ratios (SNRs) of point-source clusters on a convolved stellar density ... See full document

... Abstract. For some time the Milky Way has been understood as a barred disk galaxy. Star count observations have provided evidence for two bars at apparently different orientations, the boxy bulge and a long ... See full document

... H II Region Discovery Survey is a survey of the third and fourth quadrants of the Galactic plane that will detect radio recombination line ( RRL ) and continuum emission at cm-wavelengths from ... See full document

... The double cluster is sometimes considered to be the core of the Per OB1 association. Humphreys [22] identi- fied 105 members of the association within longitude range from 132˚ to 136˚ and latitude from −5˚ to −2.5˚, at ... See full document

... the Galactic Center – one in the first quadrant of longitude (QI) and another in the fourth (QIV) [2, ...in Quadrant I coincidentally includes an area with many HII regions, while the ... See full document

... the Galactic Cepheids are bright enough to be detected on the OGLE subtracted images, fainter RR Lyrae stars located farther in the halo are certainly missed in our preselected sample of analyzed ... See full document

... exactly which Galactic polar angles θ the observations of Williams et al. (2017) correspond to, but most likely a range of angles is used in order to get enough of the relatively rare high-velocity stars that are ... See full document

... Electrophysiological investigations have shown that the giant cell in the right upper quadrant of the abdominal ganglia RGC and the giant cell of the left pleural ganglion LGC have axona[r] ... See full document

... Hydra II) are mainly located in the region of the Oo-intermediate and Oo II ...the Milky Way was formed by the accretion of small sub-structures as expected by the LCDM cosmology, the ... See full document

... The results from the Hipparcos mission are a powerful demonstration of the value of high accuracy all-sky astrometry for studies of the structure and formation history of the Milky Way. The results from the ... See full document

... This essay is a revised version of two oral presentations, the first offered at the Distinguished Lecture Series, Uni- versity of Toronto, in January 2006, and the second at the Honouring Spi- derwoman Conference, Native ... See full document

... The prominent oval of warm dust (left of center in the lower panel of Fig. 5) is a very young 30 pc diameter super- bubble (the “Galactic Center Bubble” or GCB) whose inte- rior contains the massive, 3 to 5 My old ... See full document

... Three of the observed stellar populations, however, contain a younger stellar component: the host of SN1993aa (Fig 7.1(a)), the host of SN2008bt (Fig 7.1(c)) and the host of SN2008ca (Fig 7.1(d)). The spectra of these ... See full document

... Convincing observational support for dark matter begins with the publication by Rubin and Ford [1] concerning unexpected galactic rotation curves. These observations, soon followed by others [2], provide strong ... See full document