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(abridged) Context. The origin of hot exozodiacal dust and its connection with outer dust reservoirs remains unclear. Aims. We aim to explore the possible connection between hot exozodiacal dust and warm dust reservoirs (> 100 K) in…

(Abridged) Thirty-three objects with possible origins beyond the Kuiper Belt edge, very high inclinations, very large semi-major axes or large perihelion distances were observed to determine their surface colors. All three objects that have…

地球与行星天体物理 · 物理学 2015-05-18 Scott S. Sheppard

It is well known that some Main Belt asteroids show comet-like features. A representative example is the first known Main Belt comet 133P/(7968) Elst-Pizarro. If the mechanisms causing this activity are too weak to develop visually evident…

地球与行星天体物理 · 物理学 2014-01-23 S. Cikota , J. L. Ortiz , A. Cikota , N. Morales , G. Tancredi

Methods: We observed the high-mass hot core region G351.77-0.54 with ALMA and more than 16km baselines. Results: At a spatial resolution of 18/40au (depending on the distance), we identify twelve sub-structures within the inner few thousand…

太阳与恒星天体物理 · 物理学 2019-01-16 H. Beuther , A. Ahmadi. J. C. Mottram , H. Linz , L. T. Maud , Th. Henning , R. Kuiper , A. J. Walsh , K. G. Johnston , S. N. Longmore

The study of cometary composition is important for understanding our solar system's early evolutionary processes. Carbon dioxide (CO2) is a common hypervolatile in comets that can drive activity but is more difficult to study than other…

地球与行星天体物理 · 物理学 2024-01-03 Mikayla R. Huffman , Adam J. McKay , Anita L. Cochran

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…

Recent observations have suggested that there is water ice present on the surfaces of 24 Themis and 1 Ceres. We present upper limits on the H$_2$O production rate on these bodies derived using a search for [OI]6300 Angstrom emission. For…

地球与行星天体物理 · 物理学 2017-02-22 Adam J. McKay , Dennis Bodewits , Jian-Yang Li

Evidence for plumes of water on Europa has previously been found using the Hubble Space Telescope (HST) using two different observing techniques. Roth et al. (2014) found line emission from the dissociation products of water. Sparks et al.…

The formation of the largest objects in the Kuiper belt, with measured densities of ~1.5 g cm-3 and higher, from the coagulation of small bodies, with measured densities below 1 g cm-3 is difficult to explain without invoking significant…

地球与行星天体物理 · 物理学 2015-06-17 Michael E. Brown

Optical observations of the Oort cloud comet C/2017 K2 (PANSTARRS) show that its activity began at large heliocentric distances (up to 35 au), which cannot be explained by either the sublimation or the crystallization of water ice.…

地球与行星天体物理 · 物理学 2021-06-23 Bin Yang , David Jewitt , Yuhui Zhao , Xuejian Jiang , Quanzhi Ye , Ying-Tung Chen

Object 1I/2017 U1 (`Oumuamua) is the first interstellar small body ever discovered in the solar system. By the time of discovery, it had already passed perihelion. To investigate the behavior of `Oumuamua around perihelion, we searched for…

地球与行星天体物理 · 物理学 2020-01-08 Man-To Hui , Matthew M. Knight

A one dimensional sublimation model for cometary nuclei is used to derive size limits for the nuclei of sungrazing comets, and to estimate oxygen ion fluxes at 1 AU from their evaporation. Given that none of the ~300 sungrazers detected by…

天体物理学 · 物理学 2009-11-07 M. Iseli , M. Kueppers , W. Benz , P. Bochsler

We report the discovery of star formation activity in perhaps the most distant molecular cloud in the extreme outer galaxy. We performed deep near infrared imaging with the Subaru 8.2 m telescope, and found two young embedded clusters at…

星系天体物理 · 物理学 2015-06-23 Natsuko Izumi , Naoto Kobayashi , Chikako Yasui , Alan T. Tokunaga , Masao Saito , Satoshi Hamano

We investigated the physical properties of the comet-like objects 107P/(4015) Wilson--Harrington (4015WH) and P/2006 HR30 (Siding Spring; HR30) by applying a simple thermophysical model (TPM) to the near-infrared spectroscopy and broadband…

地球与行星天体物理 · 物理学 2024-01-15 Yoonsoo P. Bach , Masateru Ishiguro , Fumihiko Usui

We measure H$_2$ temperatures and column densities across the Orion BN/KL explosive outflow from a set of thirteen near-IR H$_2$ rovibrational emission lines observed with the TripleSpec spectrograph on Apache Point Observatory's 3.5-meter…

星系天体物理 · 物理学 2018-04-25 Allison Youngblood , Kevin France , Adam Ginsburg , Keri Hoadley , John Bally

Context: A large number of the small and the short-lived EUV brightenings have been detected in the quiet Sun (QS) over the past three years, by the High Resolution Imager of the Extreme Ultraviolet Imager (HRIEUV) on board Solar Orbiter.…

太阳与恒星天体物理 · 物理学 2024-08-09 A. Dolliou , S. Parenti , K. Bocchialini

We present the results of the study of the close binary UU Cassiopeiae based on previously published multi wavelength photometric and spectroscopic data. Based on eclipse timings of the last 117 years, we find an improved orbital period of…

太阳与恒星天体物理 · 物理学 2020-10-28 R. E. Mennickent , G. Djurašević , I. Vince , J. Garcés , P. Hadrava , M. Cabezas , J. Petrović , M. I. Jurkovic , D. Korčáková , H. Markov

We present an observational and dynamical study of newly discovered main-belt comet 313P/Gibbs. We find that the object is clearly active both in observations obtained in 2014 and in precovery observations obtained in 2003 by the Sloan…

We have used two robotic telescopes to obtain time-series high-resolution spectroscopy and V I and/or by photometry for a sample of 60 active stars. Orbital solutions are presented for 26 SB2 and 19 SB1 systems with unprecedented phase…

太阳与恒星天体物理 · 物理学 2015-06-11 K. G. Strassmeier , M. Weber , T. Granzer , S. Järvinen

Recent stellar occultations have allowed accurate instantaneous size and apparent shape determinations of the large Kuiper belt object (50000)~Quaoar and the detection of two rings with spatially variable optical depths. In this paper we…

地球与行星天体物理 · 物理学 2024-02-22 C. Kiss , T. G. Müller , G. Marton , R. Szakáts , A. Pál , L. Molnár , E. Vilenius , M. Rengel , J. L. Ortiz , E. Fernández-Valenzuela