ISM 2014 For over a decade, ISM has been an internationally renowned forum for researchers and practitioners to develop solutions and exchange ideas in emerging multimedia research and applications. In January 2015, the authors of the top ISM 2014 papers were invited to submit extended versions of their papers (with at least 30 percent new material) to this special issue. After a rigorous peer-...

We report on the detection of four rotating massive disks in two regions of high-mass star formation. The disks are perpendicular to known bipolar outflows and turn out to be unstable but long lived. We infer that accretion onto the embedded (proto)stars must proceed through the disks with rates of∼10 M⊙ yr . Subject headings: Stars: formation – Radio lines: ISM – ISM: molecules – ISM: individu...

A model of ‘integrated scientific method’ (ISM) was constructed as a framework for describing the process of science in terms of activities (formulating a research problem, and inventing and evaluating actions — such as selecting and inventing theories, evaluating theories, designing experiments, and doing experiments — intended to solve the problem) and evaluation criteria (empirical, conceptu...

Three Gram-negative, rod-shaped, aerobic bacteria that were capable of degrading dimethylsulfoniopropionate (DMSP) were isolated from marine waters. These isolates (DSS-3(T), DSS-10 and ISM(T)) exhibited the ability to demethylate and cleave DMSP, as well as to degrade other sulfur compounds related to DMSP that are cycled in marine environments. Intracellular poly-beta-hydroxybutyrate inclusio...

Penelitian ini bertujuan untuk mendeskripsikan strategi yang perlu diterapkan peningkatan Kesejahteraan Masyarakat di Kecamatan maiwa Kabupaten Enrekang.Penelitian dilaksanakan pada bulan Agustus sampai September 2020 Maiwa menggunakan metode Interpretative Struktural Modeling (ISM).Penelitian dengan ISM tidak membutuhkan sampel besar, sehingga tetapkan sebanyak 15 orang.Penelitian data primer ...

We use two 4.5μm Spitzer (IRAC) maps of the NGC 1333 region taken over a ∼ 7 yr interval to determine proper motions of its associated outflows. This is a first, successful attempt at obtaining proper motions of stellars outflow from Spitzer observations. For the outflow formed by the HerbigHaro objects HH7, 8 and 10, we find proper motions of ∼ 9-13 km s−1, which are consistent with previously...

We present the radial velocity structure of the molecular hydrogen outflows associated to the star forming region Cepheus A. This structure is derived from the doppler shift of the H2 v=1–0 S(1) emission line obtained by Fabry–Pérot spectroscopy. The East and West regions of emission, called Cep A (E) and Cep A (W), show radial velocities in the range of -20 to 0 km s with respect to the molecu...

The iron depletion level and the gas-phase iron abundance in the hot (∼ 106 K) interstellar medium (ISM) are critical to our understanding of its energy balance as well as the thermal sputtering, cooling, and heating processes of dust grains. Here we report on the first detection of the Fe XVII absorption line at 15.02 Å from the hot ISM in the spectrum of the low mass X-ray binary 4U 1820–303 ...

A local turbulence model is developed to study energy cascades in the interstellar medium (ISM) based on self-consistent two-dimensional fluid simulations. The model describes a partially ionized magnetofluid interstellar medium (ISM) that couples a neutral hydrogen fluid with a plasma primarily through charge exchange interactions. Charge exchange interactions are ubiquitous in warm ISM plasma...