Results 71 to 80 of about 2,372 (181)
ABSTRACT Mount Erciyes, the largest active volcano of Central Anatolia (Turkey), erupted explosively during the Holocene, producing the Karagüllü, Perikartin and Dikkartin tuff rings. Even though major cities like Kayseri and its ~1 million residents sit directly on these pyroclastic deposits, the timing and magnitude of the explosive eruptions have ...
Ivan Sunyé‐Puchol +12 more
wiley +1 more source
Bubbles and jets in the center of M51
Optical and radio observations of the nucleus of the galaxy M51 are presented. The observations show that M51 appears to have a bidirectional jet which emanates from the nucleus and interacts with the surrounding interstellar medium. H-alpha + forbidden N II monochromatic photographs and VLA 20 cm and 6 cm radio maps reveal a bright, resolved cloud and
H. C. Ford +4 more
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EXTENDED MARKETING MIX (7Ps) AND HRM RECRUITING. HOW TO SELL A JOB
The need to merge marketing and human resource management gained momentum in the last two decades. The paper addresses the extended marketing mix, or the 7Ps of marketing, identifies and operationalize specific HRM components that fit this framework ...
Aurelian SOFICĂ, Smaranda COSMA
doaj +1 more source
An intermediate‐mass black hole candidate in M51? [PDF]
AbstractWe present the current results of an investigation into M51 ULX‐7, using archival data from XMM‐Newton, Chandra and NuSTAR, and optical and radio data from HST and VLA. The source has a consistently hard power‐law X‐ray spectrum and high short‐term variability.
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pages, LaTeX document. For hardcopy with figures contact BEST@IASSNS.BITNET.
Rix, Hans-Walter, Rieke, Marcia J.
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Context. Molecular clouds form stars from the interstellar medium via gravitational collapse, following a sequence from low-density gas to high-density cores and eventually the formation of stars. In classical density wave theory, gas clouds orbiting the
Greve Minou +19 more
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The Star Cluster Population of M51
We present the age and mass distribution of star clusters in M51. The structural parameters are found by fitting cluster evolution models to the spectral energy distribution consisting of 8 HST-WFPC2 pass bands. There is evidence for a burst of cluster formation at the moment of the second encounter with the companion NGC5195 (50-100 Myr ago) and a ...
Gieles, M, Bastian, N, Lamers, HJGLM
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The cold and hot interstellar medium in star-forming galaxies resembles the reservoir for star formation and associated heating by stellar winds and explosions during stellar evolution, respectively.
Chunyi Zhang, Junfeng Wang, Tian-Wen Cao
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The Whirlpool Galaxy is a well-studied grand design galaxy with two major spiral arms, and a large satellite NGC 5195. The arms both show long uniform sections with perturbations (“kinks” or sharp turns) in specific regions.
Joan Font +4 more
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Aims: Structured knowledge on the combined effect of various positions of femoral and tibial tunnels in reconstruction of the anterior cruciate ligament (ACL) on knee range of motion, rotatory stability, and anterior translatory laxity is limited.
Salameh Eljaja +4 more
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