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Narrow-band H$\alpha$ and [N {\sc ii}] images and high-dispersion spatially-resolved echelle spectroscopy of the planetary nebula NGC 6891 are presented. These observations show a great wealth of structures. The bright central nebula is…

天体物理学 · 物理学 2009-10-31 M. A. Guerrero , L. F. Miranda , A. Manchado , R. Vazquez

Atmospheric circulation patterns derived from multi-spectral remote sensing can serve as a guide for choosing a suitable entry site for a future in situ probe mission. Since the Voyager-2 flybys in the 1980s, three decades of observations…

地球与行星天体物理 · 物理学 2020-03-11 Leigh N. Fletcher , Imke de Pater , Glenn S. Orton , Mark D. Hofstadter , Patrick G. J. Irwin , Michael Roman , Daniel Toledo

Interstellar interlopers are bodies formed outside of the solar system but observed passing through it. The first two identified interlopers, 1I/`Oumuamua and 2I/Borisov, exhibited unexpectedly different physical properties. 1I/`Oumuamua…

地球与行星天体物理 · 物理学 2022-09-20 David Jewitt , Darryl Z. Seligman

This paper addresses the fundamental science question: "How does solar wind energy flow through the Earth's magnetosphere, how is it converted and distributed?". We need to understand how the Sun creates the heliosphere, and how the planets…

Gravity assist manoeuvres are one of the most succesful techniques in astrodynamics. In these trajectories the spacecraft comes very close to the surface of the Earth, or other Solar system planets or moons, and, as a consequence, it…

空间物理 · 物理学 2017-01-25 L. Acedo

The fate of hot Jupiters is thought to be engulfment by their host stars, the outcome of tidal orbital decay. Transit timing has revealed a few systems with apparently shrinking orbital periods, but such signals can be mimicked by light…

地球与行星天体物理 · 物理学 2025-11-20 Joshua N. Winn , Guðmundur Stefánsson

Merging event horizons of the binary black holes is investigated. While recent development of the numerical study of the binary black hole coalescence has shown that their apparent horizons can orbit for many periods, we study the orbital…

广义相对论与量子宇宙学 · 物理学 2010-01-15 Masaru Siino , Daisuke Ida

In about 6 Giga years our Sun will evolve into a red giant and finally end its life as a white dwarf. This stellar metamorphosis will occur to virtually all known host stars of exo-planetary systems and is therefore crucial for their final…

地球与行星天体物理 · 物理学 2020-07-29 María Paula Ronco , Matthias R. Schreiber , Cristian A. Giuppone , Dimitri Veras , Jorge Cuadra , Octavio M. Guilera

The gravitational wave window onto the universe will open in roughly five years, when Advanced LIGO and Virgo achieve the first detections of high frequency gravitational waves, most likely coming from compact binary mergers.…

天体物理仪器与方法 · 物理学 2015-06-03 Joan Centrella , Samaya Nissanke , Roy Williams

We discuss two multiple star systems that host known exoplanets: HD 2638 and 30 Ari B. Adaptive optics imagery revealed an additional stellar companion to both stars. We collected multi-epoch images of the systems with Robo-AO and the…

Massive, evolved stars play a crucial role in the metal-enrichment, dust budget, and energetics of the interstellar medium, however, the details of their evolution are uncertain because of their rarity and short lifetimes before exploding…

太阳与恒星天体物理 · 物理学 2016-02-24 Ryan M. Lau , Matthew J. Hankins , Terry L. Herter , Mark R. Morris , Elisabeth A. C. Mills , Michael E. Ressler

The Cepheid AW Per is a component in a multiple system with a long period orbit. The radial velocities of Griffin (2016) cover the 38 year orbit well. An extensive program of interferometry with the CHARA array is reported here, from which…

Historically, there is no doubt that the early years of the USSR space program put them way ahead of the competition (the USA). Nonetheless, although this was not what the Russians wished to present to the world, the interplanetary…

地球与行星天体物理 · 物理学 2025-06-23 Adam Hibberd

We have learned recently that the inner halo of the Milky Way contains a kinematically coherent component (Gaia-Enceladus) from a significant merger 10 Gyrs ago. By contrast the inner halo (defined to exclude the Magellanic Stream) contains…

星系天体物理 · 物理学 2019-03-20 Jeremy Mould

We report new mid-eclipse times of the short-period sdB/dM binary HW Vir, which differ substantially from the times predicted by a previous model. The proposed orbits of the two planets in that model are found to be unstable. We present a…

太阳与恒星天体物理 · 物理学 2015-06-05 K. Beuermann , S. Dreizler , F. V. Hessman , J. Deller

HERA is taking data since 1992; after a shutdown in 2000, data taking has restarted in 2002 with a five-fold increase in the luminosity. The first running period is referred to as HERA-I, whereas the second one is referred to as HERA-II. In…

高能物理 - 实验 · 物理学 2007-05-23 Andrea Parenti

Jupiter's banded appearance may appear unchanging to the casual observer, but closer inspection reveals a dynamic, ever-changing system of belts and zones with distinct cycles of activity. Identification of these long-term cycles requires…

地球与行星天体物理 · 物理学 2017-08-18 L. N. Fletcher

The universe goes through several phase transitions during its formative stages. Cosmic reionization is the last of them, where ultraviolet and X-ray radiation escape from the first generations of galaxies heating and ionizing their…

宇宙学与河外天体物理 · 物理学 2019-07-17 John H. Wise

We announce the discovery of a planetary system with 7 transiting planets around a Kepler target, a current record for transiting systems. Planets b, c, e and f are reported for the first time in this work. Planets d, g and h were…

地球与行星天体物理 · 物理学 2015-06-17 J. Cabrera , Sz. Csizmadia , H. Lehmann , R. Dvorak , D. Gandolfi , H. Rauer , A. Erikson , C. Dreyer , Ph. Eigmueller , A. Hatzes

The heliosphere is formed due to interaction between the solar wind (SW) and local interstellar medium (LISM). The shape and position of the heliospheric boundary, the heliopause, in space depend on the parameters of interacting plasma…

太阳与恒星天体物理 · 物理学 2017-08-16 N. V. Pogorelov , J. Heerikhuisen , V. Roytershteyn , L. F. Burlaga , D. A. Gurnett , W. S. Kurth
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