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相关论文: Episodic Ejection from Active Asteroid 311P/PANSTA…

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AX J0049.4-7323 is a Be/X-ray binary that shows an unusual and poorly understood optical variability that consists of periodic and bright optical outbursts, simultaneous with X-ray outbursts, characterised by a highly asymmetric profile.…

高能天体物理现象 · 物理学 2019-01-23 L. Ducci , C. Malacaria , P. Romano , L. Ji , E. Bozzo , I. Saathoff , A. Santangelo , A. Udalski

We have measured gas and stellar velocity dispersions in 5 circumnuclear starforming regions (CNSFRs) and the nucleus of the barred spiral galaxy NGC 3351. The stellar dispersions have been obtained from high resolution spectra of the CaT…

Ejection of large boulder-like debris is a vigorous form of cometary activity that is unlikely induced by water ice out-gassing alone but rather associated with the sublimation of super-volatile ices. Though perceived on several comets,…

地球与行星天体物理 · 物理学 2024-01-31 Xian Shi , Xuanyu Hu , Jessica Agarwal , Carsten Güttler , Martin Rose , Horst Uwe Keller , Marco Fulle , Jakob Deller , Holger Sierks

The nuclei of active comets emit molecules anisotropically from discrete vents. As the nucleus rotates, we expect to observe periodic variability in the molecular emission line profiles, which can be studied through mm/submm spectroscopy.…

A sequence of events, dominated by two outbursts and ending with the preperihelion disintegration of comet C/2017 S3, is examined. The onset times of the outbursts are determined with high accuracy from the light curve of the nuclear…

地球与行星天体物理 · 物理学 2019-01-30 Zdenek Sekanina , Rainer Kracht

Observation of fast radio bursts (FRBs) are rising very quickly with the advent of specialised instruments and surveys, and it has recently been shown that some of them repeat quasi-periodically. In particular, evidence of a $P=16.35$ day…

高能天体物理现象 · 物理学 2021-09-23 Guillaume Voisin , Fabrice Mottez , Philippe Zarka

Studying small near-Earth asteroids is important to understand their dynamical histories and origins as well as to mitigate the damage of the asteroid impact to the Earth. We report the results of multicolor photometry of the tiny…

We report on accurate $BVR_{c}$ observations of (6478) Gault, a 5-6 km diameter inner main-belt asteroid in the Phocaea family, notable for its sporadic, comet-like ejection of dust. This curious behavior has been mainly interpreted as…

地球与行星天体物理 · 物理学 2020-01-28 Albino Carbognani , Alberto Buzzoni

We have performed a study of the characteristics of the circumstellar environment of the binary object HD101584, that provides information on a likely evolutionary scenario. We have obtained and analysed ALMA observations, complemented with…

太阳与恒星天体物理 · 物理学 2019-04-03 H. Olofsson , T. Khouri , M. Maercker , P. Bergman , L. Doan , D. Tafoya , W. H. T. Vlemmings , E. M. L. Humphreys , M. Lindqvist , L. Nyman , S. Ramstedt

Comet 7P/Pons-Winnecke was observed from the Calar Alto Observatory (Spain) for four months during the 2021 inbound apparition. Broad-band visible images were taken between 1.71 and 1.25 AU pre-perihelion, while long-slit spectrophotometric…

地球与行星天体物理 · 物理学 2025-03-18 Irene Mariblanca-Escalona , Luisa M. Lara , Fernando Moreno , Pedro J. Gutiérrez , Marçal Evangelista-Santana

The nuclear rotation curve of M31, as observed by the Hubble Space Telescope Faint Object Camera Spectrograph, shows a significant disturbance coinciding with the off-center brightness peak, P1. This +/- 60 km/s feature is distinguished by…

天体物理学 · 物理学 2009-10-31 Thomas S. Statler

We performed a monitoring observation of a Jupiter-Family comet, 17P/Holmes, during its 2014 perihelion passage to investigate its secular change in activity. The comet has drawn the attention of astronomers since its historic outburst in…

We present an update to the first white-light detections of a dust trail observed closely following the orbit of asteroid (3200) Phaethon, as seen by the Wide-field Imager for Parker Solar Probe (WISPR) instrument on the NASA Parker Solar…

We present high spatial resolution mid- and far-infrared images of the Vega debris disk obtained with the Multiband Imaging Photometer for Spitzer (MIPS). The disk is well resolved and its angular size is much larger than found previously.…

Stellar magnetic activity, just like that of the Sun, manifests itself in the form of flares and spots on the surface of the star. In the solar case, the largest flares originate from large active regions. In this work, we present a study…

太阳与恒星天体物理 · 物理学 2021-12-01 Alexandre Araújo , Adriana Valio

The abundance and distribution of metal in asteroid surfaces can be constrained from thermal emission measurements at radio wavelengths, informing our understanding of planetesimal differentiation processes. We observed the M-type asteroid…

地球与行星天体物理 · 物理学 2024-09-20 Katherine de Kleer , Saverio Cambioni , Bryan Butler , Michael Shepard

We observed stars with variable radial velocities to determine their spectroscopic orbits. Velocities of 132 targets taken over a time span reaching 30 years are presented. They were measured with the correlation radial velocity…

太阳与恒星天体物理 · 物理学 2019-06-12 J. Sperauskas , V. Deveikis , A. Tokovinin

We conducted a polarimetric observation of the fast-rotating near-Earth asteroid (1566) Icarus at large phase (Sun-asteroid-observer's) angles $\alpha$= 57 deg--141deg around the 2015 summer solstice. We found that the maximum values of the…

The detection of circumstellar atomic hydrogen (\ion{H}{1}) via the 21\,cm line remains a persistent challenge in planetary nebula (PN) studies, primarily due to contamination from ubiquitous interstellar \ion{H}{1} 21\,cm emission. In this…

A morphological and photometric analysis of the naked-eye long-period comet C/2022 E3 (ZTF) before perihelion is presented in this study. The observation images taken by the Zwicky Transient Facility survey telescope from July 2022 to…

地球与行星天体物理 · 物理学 2024-05-27 Bin Liu , Xiaodong Liu