scholarly journals Solvent-tuning the collapse and helix formation time scales of λ6-85*

2006 ◽  
Vol 15 (11) ◽  
pp. 2596-2604 ◽  
Author(s):  
Charles Dumont ◽  
Yoshitaka Matsumura ◽  
Seung Joong Kim ◽  
Jinsong Li ◽  
Elena Kondrashkina ◽  
...  
Keyword(s):  
Time Scales ◽  
Formation Time ◽  
Helix Formation

1P109 Solvent-tuning collapse and helix formation time scales of λ^*_6-85(3. Protein folding and misfolding (I),Poster Session,Abstract,Meeting Program of EABS & BSJ 2006)

2006 ◽  
Vol 46 (supplement2) ◽  
pp. S174
Author(s):  
Charles Dumont ◽  
Yoshitaka Matsumura ◽  
Seung J. Kim ◽  
Jinsong Li ◽  
Elena Kondrashkina ◽  
...  
Keyword(s):  
Protein Folding ◽  
Time Scales ◽  
Poster Session ◽  
Formation Time ◽  
Meeting Program ◽  
Helix Formation

scholarly journals Photometric Studies of the Extreme SMC Wing

1980 ◽  
Vol 85 ◽  
pp. 353-355 ◽  
Author(s):  
William E. Kunkel
Keyword(s):  
Star Formation ◽  
Time Scales ◽  
Formation Time ◽  
Stellar Systems ◽  
Tidal Disruption ◽  
Tidal Interaction ◽  
Magellanic Stream

Among the currently interesting problems of interpreting the Magellanic Stream as an instance of tidal disruption is that of finding some demonstrable phenomenon in the makeup of the involved material that parallels the better known cases of tidal interaction, as for example NGC4038/39, where the dynamic and star-formation time scales are in agreement (Schweizer 1977). The observational problems that beset the interpretation of the Magellanic Stream are numerous (Mathewson and Schwartz 1976, Kunkel 1979, Bregman 1979), and the marked difference between the composition of the Stream (evidenced purely through HI) and the stellar systems (at least 80 percent stars) is among the outstanding dilemmas remaining. Finding some counterpart in the Magellanic scene comparable to the better recognized instances of tidal interaction may go some way towards clarifying a perplexing situation.

scholarly journals Dancing to changa: a self-consistent prediction for close SMBH pair formation time-scales following galaxy mergers

2018 ◽  
Vol 475 (4) ◽  
pp. 4967-4977 ◽  
Author(s):  
M Tremmel ◽  
F Governato ◽  
M Volonteri ◽  
T R Quinn ◽  
A Pontzen
Keyword(s):  
Time Scales ◽  
Pair Formation ◽  
Formation Time ◽  
Galaxy Mergers ◽  
Self Consistent

scholarly journals The noble gas isotope record of hydrocarbon field formation time scales

2017 ◽  
Vol 471 ◽  
pp. 141-152 ◽  
Author(s):  
Igor N. Tolstikhin ◽  
Chris J. Ballentine ◽  
Boris G. Polyak ◽  
Edward M. Prasolov ◽  
Olga E. Kikvadze
Keyword(s):  
Time Scales ◽  
Noble Gas ◽  
Formation Time ◽  
Isotope Record ◽  
Noble Gas Isotope ◽  
Field Formation ◽  
Hydrocarbon Field

scholarly journals Formation time-scales for high-mass X-ray binaries in M33

2018 ◽  
Vol 479 (3) ◽  
pp. 3526-3544 ◽  
Author(s):  
Kristen Garofali ◽  
Benjamin F Williams ◽  
Tristan Hillis ◽  
Karoline M Gilbert ◽  
Andrew E Dolphin ◽  
...  
Keyword(s):  
Time Scales ◽  
Formation Time ◽  
High Mass ◽  
X Ray ◽  
X Ray Binaries

scholarly journals New Low-mass Accretors in the Scorpius-Centaurus OB Association

2015 ◽  
Vol 10 (S314) ◽  
pp. 58-62
Author(s):  
Simon J. Murphy ◽  
Warrick A. Lawson ◽  
Joao Bento
Keyword(s):  
Time Scales ◽  
Planet Formation ◽  
Formation Time ◽  
Lower Mass ◽  
Circumstellar Material ◽  
Hα Emission ◽  
Low Mass

AbstractWe describe the serendipitous discovery of two new lithium-rich M5 members of the Scorpius-Centaurus OB Association (Sco-Cen). Both stars exhibit large 12 and 22 μm excesses and strong, variable Hα emission which we attribute to accretion from circumstellar discs. Such stars are thought to be incredibly rare at the ~16 Myr median age of much of Sco-Cen. The serendipitous discovery of two accreting stars hosting large quantities of circumstellar material may be indicative of a sizeable age spread in Sco-Cen, or further evidence that disc dispersal and planet formation time-scales are longer around lower-mass stars.

scholarly journals Mapping collinear in-medium parton splittings

2020 ◽  
Vol 80 (1) ◽  
Author(s):  
Fabio Domínguez ◽  
José Guilherme Milhano ◽  
Carlos A. Salgado ◽  
Konrad Tywoniuk ◽  
Víctor Vila
Keyword(s):  
Phase Space ◽  
Radiation Pattern ◽  
Time Scales ◽  
Transport Coefficient ◽  
Formation Time ◽  
Close Correspondence ◽  
Classical Description ◽  
Theoretical Support

AbstractWe map the spectrum of $$1\rightarrow 2$$1→2 parton splittings inside a medium characterized by a transport coefficient $${\hat{q}}$$q^ onto the kinematical Lund plane, taking into account the finite formation time of the process. We discuss the distinct regimes arising in this map for in-medium splittings, pointing out the close correspondence to a semi-classical description in the limit of hard, collinear radiation with short formation times. Although we disregard any modifications of the original parton kinematics in course of the propagation through the medium, subtle modifications to the radiation pattern compared to the vacuum baseline can be traced back to the physics of color decoherence and accumulated interactions in the medium. We provide theoretical support to vacuum-like emissions inside the medium by delimiting the regions of phase space where it is dominant, identifying also the relevant time-scales involved. The observed modifications are shown to be quite general for any dipole created in the medium.

scholarly journals Observational diagnostics of elongated planet-induced vortices with realistic planet formation time-scales

2018 ◽  
Vol 482 (3) ◽  
pp. 3609-3621 ◽  
Author(s):  
Michael Hammer ◽  
Paola Pinilla ◽  
Kaitlin M Kratter ◽  
Min-Kai Lin
Keyword(s):  
Time Scales ◽  
Planet Formation ◽  
Formation Time
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