نتایج جستجو برای: works and companions

تعداد نتایج: 16834326  

2010
O. Absil

Aims. We search for low-mass companions in the innermost region (<300 mas, i.e., 6 AU) of the β Pic planetary system. Methods. We obtained interferometric closure phase measurements in the K-band with the VLTI/AMBER instrument used in its medium spectral resolution mode. Fringe stabilization was provided by the FINITO fringe tracker. Results. In a search region of between 2 and 60 mas in radius...

2004
E. Guenther

We present an overview of our ongoing systematic search for wide (sub)stellar companions around the stars known to host rad-vel planets. By using a relatively large field of view and going very deep, our survey can find all directly detectable stellar and massive brown dwarf companions (m>40 MJup) within a 1000 AU orbit.

2010
Naveed Ahmad

Juridical English, judicial opinions written by judges of higher judiciary, is an extremely important genre for legal discourse community. In situations where learners’ first language is other than English, law students and recent law graduates in the profession of law reportedly find it hard to cope with a variety of tasks they are required to perform while reading judicial opinions/cases. The...

Journal: :BJET 2007
Eric Deeson

Will reading habit influence your life? Many say yes. Reading cases on global e learning practices successes and pitfalls is a good habit; you can develop this habit to be such interesting way. Yeah, reading habit will not only make you have any favourite activity. It will be one of guidance of your life. When reading has become a habit, you will not make it as disturbing activities or as borin...

Journal: :iJET 2008
Marius Dieperink

This paper reports on a case study that explored the effect of an English-as-Second Language (ESL) computer program at Tshwane University of Technology (TUT), South Africa. The case study explored participants’ perceptions, attitudes and beliefs regarding the ESL reading enhancement program, Reading ExcellenceTM. The study found that participants experienced the program in a positive light. The...

1999
William D. Cochran Michel Mayor

The mass distribution of substellar companions exhibits a steep rise for masses below 5 MJ. Thus, the 14 companions having Msin i = 0.5 { 5 MJ are considered the best candidate planets around main sequence stars. The occurrence of such planets within 3 AU is 4%, but 2/3 of them orbit within just 0.3 AU. This \pile up" of planets near stars suggests that inward orbital migration occurred after f...

Journal: :Research in Astronomy and Astrophysics 2022

The development of large-scale time-domain surveys provides an opportunity to study the physical properties as well evolutionary scenario B-type subdwarfs (sdB) and M-type dwarfs (dM). Here, we obtained 33 sdB+dM eclipsing binaries based on Zwicky Transient Facility (ZTF) light curves $Gaia$ early data release 3 (EDR3) parallaxes. By using PHOEBE code for curve analysis, obtain probability dist...

2001
Henrique R. Schmitt

We analyze the idea that nuclear activity, either AGN or star formation, can be triggered by interactions, studying the percentage of active, HII and quiescent galaxies with companions. Our sample was selected from the Palomar survey, and avoids selection biases faced by previous studies. This sample was split into 5 different groups, Seyfert galaxies, LINERs, transition galaxies, HII galaxies ...

2013
Ida J Korfage Suzanne Audrey Tony Hak Jane M Blazeby Julian Abel Rona Campbell

OBJECTIVES Patients are often accompanied by family or companions during consultations, but little is known about how this might influence the process. We explored how the presence of a companion in a consultation contributes to communication and the decision-making process. DESIGN Observational study. SETTING A teaching hospital and a district general hospital in south-west England. PART...

1999
E Athanassoula

Disc galaxies can be substantially modified by close encounters and mergers, since their discs are very responsive components. Close interactions can be held responsible for the formation of bridges and tails, as well as for the formation of some bars, asymmetries and grand design spirals. Bound clumps can form in the tails, due to self-gravity, and could evolve to dwarf galaxies. Off-centering...

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