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相关论文: Lensing of Invisible Stars by Brown Dwarfs

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The presence of brown dwarfs in the dark galactic halo could be detected through their gravitational lensing effect and experiments under way monitor about one million stars to observe a few lensing events per year. We show that if the…

天体物理学 · 物理学 2007-05-23 Paul Baillon , Alain Bouquet , Yannick Giraud-Héraud , Jean Kaplan

Experiments are looking for diffuse brown dwarfs in the dark galactic halo through the gravitational lens effect. If brown dwarfs are clumped in dark clusters, the event rate is not changed, but events are spatially clustered, and stars…

天体物理学 · 物理学 2007-05-23 Alain Bouquet , Jean Kaplan , Jean-Manuel Verschaeve

We describe a project of brown dwarf detection in the dark halo of a galaxy using the microlensing effect. We argue that monitoring pixels instead of stars could provide an enhancement in the number of detectable events. We estimate the…

天体物理学 · 物理学 2009-09-25 Alain Bouquet , Jean Kaplan , Anne-Laure Melchior , Yannick Giraud-Héraud , Paul Baillon

Gravitational lensing provides a means to measure mass that does not rely on detecting and analysing light from the lens itself. Compact objects are ideal gravitational lenses, because they have relatively large masses and are dim. In this…

天体物理仪器与方法 · 物理学 2017-06-15 A. J. Harding , R. Di Stefano , S. Lépine , J. Urama , D. Pham , C. Baker

It has been shown by Paczy\'nski that gravitational microlensing is a useful method to detect brown dwarfs in the dark halo of our galaxy. At present several experiments are carried out to monitor several million stars in the Large…

天体物理学 · 物理学 2008-02-03 Philippe Jetzer

We consider the gravitational magnification of light for binary systems containing two compact objects: white dwarfs, a white dwarf and a neutron star or a white dwarf and a black hole. Light curves of the flares of the white dwarf caused…

天体物理学 · 物理学 2009-11-07 Gregory M. Beskin , Artyom V. Tuntsov

In the cold dark matter scenario, dark matter halos are assembled hierarchically from smaller subunits. Some of these subunits are disrupted during the merging process, whereas others survive temporarily in the form of subhalos. A…

宇宙学与河外天体物理 · 物理学 2015-05-13 E. Zackrisson , T. Riehm

It is estimated that a star brighter than visual magnitude 17 is undergoing a detectable gravitational microlensing event, somewhere on the sky, at any given time. It is assumed that both lenses and sources are normal stars drawn from a…

天体物理学 · 物理学 2009-10-30 Robert J. Nemiroff

Microlensing events are now regularly being detected by monitoring the flux of a large number of potential sources and measuring the combined magnification of the images. This phenomenon could also be detected directly from the…

天体物理学 · 物理学 2009-10-28 Jordi Miralda-Escude

The status of searches for gravitational microlensing events of the stars in our galaxy and in other galaxies of the Local Group, the interpretation of the results, some theory, and prospects for the future are reviewed. The searches have…

天体物理学 · 物理学 2011-05-05 Bohdan Paczynski

Previous calculations of the rates and optical depths due to microlensing only considered resolved stars. However, if a faint unresolved star lens is close enough to a resolved star, the event will be seen by the microlensing experiments…

天体物理学 · 物理学 2007-05-23 C. Alard

If the Galaxy contains ~10^{11}M_sol in cold gas clouds of ~Jovian mass and \~AU size, these clouds will act as converging lenses for optical light, magnifying background stars at a detectable rate. The resulting light curves can resemble…

天体物理学 · 物理学 2009-10-30 B. T. Draine

A nearby star having a near-transit of a galaxy will cause a time-dependent weak lensing of the galaxy. Because the effect is small, we refer to this as weak microlensing. This could provide a useful method to weigh low-mass stars and brown…

太阳与恒星天体物理 · 物理学 2015-05-14 Jonathan Coles , Prasenjit Saha , Hans Martin Schmid

It has been shown by Paczy\'nski that gravitational microlensing is potentially a useful method for detecting the dark constituents of the halo of our galaxy, if their mass lies in the approximate domain $10^{-6} < M/M_{\odot} < 10^{-1}$.…

天体物理学 · 物理学 2008-02-03 Philippe Jetzer

Detecting compact objects by means of their gravitational lensing effect on an observed companion in a binary system has already been suggested almost four decades ago. However, these predictions were made even before the first observations…

太阳与恒星天体物理 · 物理学 2015-05-19 S. Rahvar , A. Mehrabi , M. Dominik

A substantial fraction the stellar mass attributed to galaxies is invisible: stars close to the hydrogen burning limit, brown dwarfs, white dwarfs, neutron stars and black holes. These constituents do, however, gravitationally micro-lens…

星系天体物理 · 物理学 2017-12-04 Paul L. Schechter

If the dark halo of our galaxy is made of compact objects as massive as M = 10^6 solar masses, their detection by means of ordinary microlensing searches would take a very long time as the characteristic time scale of such a lensing event,…

天体物理学 · 物理学 2007-05-23 Bohdan Paczynski

The high-magnification gravitational lensing cross-section of a galaxy is enhanced significantly if a baryonic disc is embedded in its dark matter halo. We investigate the effects of a population of such disks on the probability of…

天体物理学 · 物理学 2009-10-31 Andrew W. Blain , Ole Moeller , Ariyeh H. Maller

We demonstrate that gravitational lensing can be used to discover and study planets in the habitable zones of nearby dwarf stars. If appropriate software is developed, a new generation of monitoring programs will automatically conduct a…

天体物理学 · 物理学 2008-01-11 Rosanne Di Stefano , Christopher Night

Microlensing of distant stars in the Milky Way by the nearby high proper motion stars offers a direct way to precisely measure the masses of single lower main sequence stars and brown dwarfs.

天体物理学 · 物理学 2007-05-23 B. Paczynski
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