中文
相关论文

相关论文: Nebulosities of the Symbiotic Binary R Aquarii -- …

200 篇论文

We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 130 sources and provides information on names and spectral types of optical…

天体物理学 · 物理学 2016-08-30 N. V. Raguzova , S. B. Popov

Binary central stars have long been invoked to explain the vexing shapes of planetary nebulae (PNe) despite there being scant direct evidence to support this hypothesis. Modern large-scale surveys and improved observing strategies have…

太阳与恒星天体物理 · 物理学 2015-05-30 Brent Miszalski

Active galactic nuclei (AGN) have been proposed as environments that can facilitate the capture of extreme-mass-ratio binaries and accelerate their inspiral beyond the rate expected from gravitational wave emission alone. In this work, we…

星系天体物理 · 物理学 2026-03-25 Thomas F. M. Spieksma , Enrico Cannizzaro

Planetary nebulae are traditionally considered to represent the final evolutionary stage of all intermediate-mass stars ($\sim$0.7-8Msol). Recent evidence seems to contradict this picture. In particular, since the launch of the Hubble Space…

太阳与恒星天体物理 · 物理学 2017-05-02 David Jones , Henri M. J. Boffin

Binary stars play a critical role in determining both the dynamical evolution and the observational appearance of globular star clusters. We present a summary of three talks presented at IAU JD15, reviewing the current observational and…

天体物理学 · 物理学 2007-05-23 S. L. W. McMillan , C. Pryor , E. S. Phinney

We present high-resolution ALMA Band 6 and 7 observations of the tidally disrupted protoplanetary disks of the RW Aurigae binary. Our observations reveal the presence of additional tidal streams to the previously observed tidal arm around…

We present a new analytic study of the equilibrium and stability properties of close binary systems containing polytropic components. Our method is based on the use of ellipsoidal trial functions in an energy variational principle. We…

天体物理学 · 物理学 2009-10-22 D. Lai , F. A. Rasio , S. L. Shapiro

We report our spectroscopic observations of stars belonging to the young nearby group known as the TW Hydrae association, as well as of a number of potential members of the association identified in kinematic and X-ray surveys. Multiple…

During the past decade circumbinary disks have been discovered around various young binary stars. Hydrodynamical calculations indicate that the gravitational interaction between the central binary star and the surrounding disk results in…

地球与行星天体物理 · 物理学 2015-07-15 Jan Philipp Ruge , Sebastian Wolf , Tatiana Demidova , Vladimir Grinin

We conducted sub-arcsecond near-infrared imaging observations of RNO91 with CIAO mounted on the SUBARU 8.2 m telescope. We present our JHK band data along with optical images, which when considered together reveal a complex circumstellar…

In this paper, I present and discuss some recent observational results which may have important implications for our understanding of late phases of binary evolution.

太阳与恒星天体物理 · 物理学 2018-03-14 J. Mikołajewska

Dusty protoplanetary disks surrounding young low-mass stars are the birthplaces of planets. Studies of the evolutionary timescales of such disks provide important constraints on the timescales of planet formation. Binary companions,…

太阳与恒星天体物理 · 物理学 2009-12-10 M. G. Petr-Gotzens , S. Daemgen , S. Correia

Stars are generally spherical, yet their gaseous envelopes often appear non-spherical when ejected near the end of their lives. This quirk is most notable during the planetary nebula phase when these envelopes become ionized. Interactions…

While there has been significant progress in our understanding of the origin and evolu-tion of planetary nebulae in the last 50 years, there remain several unsolved problems. These include the true 3D morphological structure of the nebulae,…

太阳与恒星天体物理 · 物理学 2026-04-28 Sun Kwok , Bruce Balick , You-Hua Chu , Bruce J. Hrivnak , Alberto López , Quentin Parker , Raghvendra Sahai , Albert Zijlstra

Observations of brown dwarfs provide important feedback on theories of atmospheres and inner structure of substellar objects. Brown dwarf binary systems furthermore offer the unique opportunity to determine the mass of individual brown…

天体物理学 · 物理学 2007-05-23 Wolfgang Brandner , Herve Bouy , Eduardo L. Martin , Stefan Umbreit

Neutron stars and stellar-mass black holes are the remnants of massive stars, which ended their lives in supernova explosions. These exotic objects can only be studied in relatively rare cases. If they are interacting with close companions…

太阳与恒星天体物理 · 物理学 2009-07-22 Stephan Geier , Uli Heber , Heinz Edelmann , Thomas Kupfer , Ralf Napiwotzki , Philipp Podsiadlowski

Results from a six year systematic observational survey on candidate eclipsing binaries with a $\delta$ delta Sct component are presented. More than a hundred systems with component(s) of A-F spectral types were observed in the frame of…

太阳与恒星天体物理 · 物理学 2015-06-25 Alexios Liakos , Panagiotis Niarchos

The study of asteroids, its composition and trajectories, has been a persistent interest in the space exploration community. In addition, they are also perceived as a great threat to life on Earth, considering the possibility of an impact…

地球与行星天体物理 · 物理学 2023-07-14 Lucas G. Meireles , Antonio F. B. de A. Prado , Maria Cecília Pereira , Cristiano F. de Melo

We have gathered a sample of 112 main-sequence stars with known debris disks. We collected published information and performed adaptive optics observations at Lick Observatory to determine if these debris disks are associated with binary or…

太阳与恒星天体物理 · 物理学 2015-06-03 David R. Rodriguez , B. Zuckerman