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Related papers: Characterizing the nucleus of comet 162P/Siding Sp…

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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,…

Observing the vibrational/rotational lines in a comet's optical spectrum requires high-resolution spectroscopy, as they are otherwise seen as a blended feature. To achieve this, we have obtained medium and high-resolution (R…

Earth and Planetary Astrophysics · Physics 2024-04-11 K Aravind , Kumar Venkataramani , Shashikiran Ganesh , Arun Surya , Thirupathi Sivarani , Devendra Sahu , Athira Unni , Anil Bhardwaj

Comet C/2017 K2 (PANSTARRS) was discovered by the Pan-STARRS1 (PS1) Survey on 2017 May 21 at a distance 16.09 au from the Sun, the second most distant discovery of an active comet. Pre-discovery images in the PS1 archive back to 2014 and…

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…

Earth and Planetary Astrophysics · Physics 2015-06-19 R. Stevenson , J. M. Bauer , E. A. Kramer , T. Grav , A. K. Mainzer , J. R. Masiero

On 3 and 4 October, 1995, we obtained high spectral resolving power (R=\lambda/\Delta\lambda = 60,000) observations of comet 122P/de Vico using the 2DCoude cross-dispersed echelle spectrograph on the 2.7-m telescope of McDonald Observatory.…

Astrophysics · Physics 2015-06-24 Anita L. Cochran , William D. Cochran

We present an analysis of the photometric data of new main belt comet P/2023 JN16 (Lemmon) observed with the 1.35-m SkyMapper telescope at Siding Spring Observatory in 2024 during July - September. The faint object showed dusty activity…

Earth and Planetary Astrophysics · Physics 2026-03-24 Serhii Borysenko , Alexander Baransky , Christopher A. Onken , Iryna Kulyk

We report observations of nine MBCs or candidate MBCs, most of which were obtained when the targets were apparently inactive. We find effective nucleus radii (assuming albedos of p_V=0.05+/-0.02) of r_n=(0.24+/-0.05) km for 238P/Read,…

We present the CoRoT light curve of the Beta Cep star HD 180642, assembled during the first long run of the space mission, as well as archival single-band photometry. Our goal is to analyse the detailed behaviour present in the light curve…

Solar and Stellar Astrophysics · Physics 2015-05-13 P. Degroote , M. Briquet , C. Catala , K. Uytterhoeven , K. Lefever , T. Morel , C. Aerts , F. Carrier , M. Auvergne , A. Baglin , E. Michel

We present analyses of Spitzer observations of 29P/Schwassmann-Wachmann 1 using 16 $\mu$m IRS "blue" peak-up (PU) and 24 $\mu$m and 70 $\mu$m MIPS images obtained on UT 2003 November 23 and 24 that characterize the Centaur's large-grain…

Type II-plateau supernovae (SNe II-P) are the classic variety of core-collapse events that result from isolated, massive stars with thick hydrogen envelopes intact at the time of explosion. Their distances are now routinely estimated…

Astrophysics · Physics 2009-11-07 Douglas C. Leonard , Shashi M. Kanbur , Choong C. Ngeow , Nial R. Tanvir

We present simultaneous, multi-colour optical light curves of the companion star to the black-widow pulsar PSR J2051-0827, obtained approximately 10 years apart using ULTRACAM and HiPERCAM, respectively. The ULTRACAM light curves confirm…

Ultra-hot Jupiters exhibit day-to-night temperature contrasts upwards of 1000 K due to competing effects of strong winds, short radiative timescales, magnetic drag, and H2 dissociation/recombination. Spectroscopic phase curves provide…

We report on the high-resolution spectroscopic observations of two planetary transits of the hot Jupiter KELT-7b ($M_{\rm p}$ $=$ 1.28 $\pm$ 0.17 M$_{\rm Jup}$, $T_{\rm eq}$ $=$ 2028 K) observed with the High Optical Resolution Spectrograph…

Aims. Rotation periods of cometary nuclei are scarce, though important when studying the nature and origin of these objects. Our aim is to derive a rotation period for the nucleus of comet C/2004 Q2 (Machholz). Methods. C/2004 Q2 (Machholz)…

Context. Breathtaking imagery recorded during the European Space Agency's Rosetta mission confirmed the bilobate nature of comet 67P/Churyumov-Gerasimenko's nucleus. Its peculiar appearance is not unique among comets. The majority of…

Earth and Planetary Astrophysics · Physics 2019-01-30 D. E. Vavilov , S. Eggl , Yu. D. Medvedev , P. B. Zatitskiy

We observed two full orbital phase curves of the transiting brown dwarf KELT-1b, at 3.6um and 4.5um, using the Spitzer Space Telescope. Combined with previous eclipse data from Beatty et al. (2014), we strongly detect KELT-1b's phase…

Earth and Planetary Astrophysics · Physics 2019-10-09 Thomas G. Beatty , Mark S. Marley , B. Scott Gaudi , Knicole D. Colon , Jonathan J. Fortney , Adam P. Showman

We report HST lightcurve observations of the New Horizons (NH) spacecraft encounter KBO (486958) 2014 MU69 acquired near opposition in July 2017. In order to plan the optimum flyby sequence the NH mission planners needed to learn as much as…

Earth and Planetary Astrophysics · Physics 2020-02-12 S. D. Benecchi , S. Porter , M. W. Buie , A. M. Zangari , A. J. Verbiscer , K. S. Noll , S. A. Stern , J. R. Spencer , A. Parker

We make the following predictions: (1) Comet 67P/Churyumov-Gerasimenko. The Secular Light Curve (SLC) of this comet exhibits a photometric anomaly in magnitude that is present in 1982, 1996, 2002 and 2009. Thus it must be real. We interpret…

Earth and Planetary Astrophysics · Physics 2015-06-19 Ignacio Ferrín

In this work, the temporal and spectral properties of the poorly studied X-ray pulsar Swift J1808.4$-$1754 were investigated in the 0.8-79 keV energy range based on the data from the NuSTAR and Swift observatories collected during the 2014…

High Energy Astrophysical Phenomena · Physics 2022-06-08 Alexander Salganik , Sergey S. Tsygankov , Alexander A. Lutovinov , Anlaug A. Djupvik , Dmitri I. Karasev , Sergey V. Molkov
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