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We carried out photometric and spectroscopic observations of comet 29P/ Schwassmann-Wachmann 1 at the SOAR 4.1-meter telescope (Chile) on August 12, 2016. This paper presents the results of only spectroscopic analysis. The spectra revealed…

地球与行星天体物理 · 物理学 2018-05-18 Oleksandra V. Ivanova , Enos Picazzio , Igor V. Luk'yanyk , Oscar Cavichia , Sergei M. Andrievsky

Spectra of comet C/2014 Q2 (Lovejoy) were taken with a low resolution spectrograph mounted on the 0.5 m telescope at the Mount Abu Infrared Observatory (MIRO), India during January to May 2015 covering the perihelion and post-perihelion…

地球与行星天体物理 · 物理学 2016-09-27 Kumar Venkataramani , Satyesh Ghetiya , Shashikiran Ganesh , U. C. Joshi , Vikrant K. Agnihotri , K. S. Baliyan

We observed Comet C/Siding Spring using the Hubble Space Telescope (HST) during its close approach to Mars. The high spatial resolution images obtained through the F689M, F775W, and F845M filters reveal the characteristics of the dust coma.…

We investigated three comets, which are active at large heliocentric distances, using observations obtained at the 6-m BTA telescope (SAO RAS, Russia) in the photometric mode of the focal reducer SCORPIO. The three comets,…

地球与行星天体物理 · 物理学 2021-02-10 Oleksandra Ivanova , Yury Skorov , Pavlo Korsun , Viktor Afanasiev , Jürgen Blum

Images and low-resolution spectra of the near-Earth Jupiter family comet (JFC) 249P/LINEAR in the visible range obtained with the instrument OSIRIS in the 10.4m Gran Telescopio Canarias on January 3, 4, 6 and February 6, 2016 are presented,…

We studied C/2025 D1 (Groeller), a long-period comet with an unprecedented perihelion distance of 14.1 au, using archival observations. The data reveals that it had been active at inbound heliocentric distances $r_{\rm H} \gtrsim 20$ au.…

地球与行星天体物理 · 物理学 2026-01-14 Man-To Hui , Robert Weryk , Marco Micheli , Sam Deen , David J. Tholen , Jianchun Shi , Xian Shi , Richard Wainscoat

We imaged Comet 252P/2000 G1 (LINEAR) (hereafter 252P) with the Hubble Space Telescope and both 252P and P/2016 BA$_{14}$ (PanSTARRS) (hereafter BA$_{14}$) with the Discovery Channel Telescope in March and April 2016, surrounding its close…

We report the result of a new Chandra observation of the black hole X-ray transient H 1705-250 in quiescence. H 1705-250 was barely detected in the new 50 ks Chandra observation. With 5 detected counts, we estimate the source quiescent…

高能天体物理现象 · 物理学 2015-06-11 Yi-Jung Yang , Albert K. H. Kong , David M. Russell , Fraser Lewis , Rudy Wijnands

We present the polarimetric results and analysis of comet C/2012 L2 (LINEAR) observed at 31$^\circ$.1 phase angle before perihelion passage. The observations of the comet were carried out using ARIES Imaging Polarimeter (AIMPOL) mounted on…

地球与行星天体物理 · 物理学 2014-12-01 P. DebRoy , H. S. Das , Biman J. Medhi

The main aim of photometrical observations of the asteroid 3200 Phaethon was searching for its low-level cometary activity (possible coma and/or dust tail) in the pre-perihelion passage. We performed observational runs with telescopes…

地球与行星天体物理 · 物理学 2019-06-05 A. Kartashova , M. Husarik , O. Ivanova , G. Kokhirova , E. Bakanas , I. Sokolov , U. Kh. Khamroev , A. A. Ibragimov

The central kiloparsec region of the Andromeda galaxy is relatively gas poor, while the interstellar medium appears to be concentrated in a ring-like structure at about 10 kpc radius. The central gas depletion has been attributed to a…

星系天体物理 · 物理学 2015-12-16 A. -L. Melchior , F. Combes

The results of the 9P/Tempel 1 CARA (Cometary Archive for Amateur Astronomers) observing campaign is presented. The main goal was to perform an extended survey of the comet as a support to the Deep Impact (DI) Mission. CCD R, I and…

The results of the photometric observations of comet C/2009 P1 (Garradd) performed at the 60-cm Zeiss-600 telescope of the Terskol observatory have been analyzed. During the observations, the comet was at the heliocentric and geocentric…

地球与行星天体物理 · 物理学 2021-01-15 A. V. Ivanova , S. A. Borisenko , M. V. Andreev

The thermal emission of comet C/2013 A1 (Siding Spring) was observed on March 31, 2013, at a heliocentric distance of 6.48 au using the PACS photometer camera of the Herschel Space Observatory. The comet was clearly active, showing a coma…

地球与行星天体物理 · 物理学 2015-01-21 Cs. Kiss , T. G. Müller , M. Kidger , P. Mattisson , G. Marton

We present a statistical analysis of 43 coronal dimming events, associated with Earth-directed CMEs that occurred during the period of quasi-quadrature of the SDO and STEREO satellites. We studied coronal dimmings that were observed above…

太阳与恒星天体物理 · 物理学 2020-06-11 Galina Chikunova , Karin Dissauer , Tatiana Podladchikova , Astrid M. Veronig

Comet 17P/Holmes underwent a massive outburst in 2007 Oct., brightening by a factor of almost a million in under 48 hours. We used infrared images taken by the Wide-Field Survey Explorer mission to characterize the comet as it appeared at a…

地球与行星天体物理 · 物理学 2015-06-19 R. Stevenson , J. M. Bauer , E. A. Kramer , T. Grav , A. K. Mainzer , J. R. Masiero

We present new near-infrared (1.1-micron) observations of the circumstellar environment of the planet-bearing star 55 Cancri. With these Hubble Space Telescope images we are unable to confirm the observation of bright scattered radiation at…

天体物理学 · 物理学 2009-10-31 G. Schneider , E. E. Becklin , B. A. Smith , A. J. Weinberger , M. Silverstone , D. C. Hines

We present initial observations of the interstellar body 2I/(2019 Q4) Borisov taken to determine its nature prior to the perihelion in 2019 December. Images from the Nordic Optical Telescope show a prominent, morphologically stable dust…

地球与行星天体物理 · 物理学 2020-01-08 David Jewitt , Jane Luu

We present an in-depth characterization of the polarimetric channel of the Large-Angle Spectrometric COronagraph LASCO-C2 onboard the Solar and Heliospheric Observatory (SoHO). The polarimetric analysis of the white-light images makes use…

太阳与恒星天体物理 · 物理学 2020-07-21 Philippe Lamy , Antoine Llebaria , Brice Boclet , Hugo Gilardy , Michael Burtin , Olivier Floyd

The release of volatiles from comets is usually from direct sublimation of ices on the nucleus, but for very or hyper-active comets other sources have to be considered to account for the total production rates. In this work, we present new…

地球与行星天体物理 · 物理学 2023-04-13 Theodore Kareta , John W. Noonan , Walter M. Harris , Alessondra Springmann