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We present ALMA CO(2-1) observations of the Seyfert 2 galaxy NGC 3281 at $\sim$ 100 pc spatial resolution. This galaxy was previously known to present a bi-conical ionised gas outflow extending to 2 kpc from the nucleus. The analysis of the…

We report high-spectral resolution observations of comet 9P/Tempel 1 before, during and after the impact on 4 July 2005 UT of the Deep Impact spacecraft with the comet. These observations were obtained with the HIRES instrument on Keck 1.…

Astrophysics · Physics 2009-11-11 Anita L. Cochran , William M. Jackson , Karen J. Meech , Micah Glaz

Extensive observations of comet C/2004 Q2 (Machholz) were carried out between August 2004 and May 2005. The images obtained were used to investigate the comet's inner coma features at resolutions between 350 and 1500 km/pixel. A photometric…

We have carried out a continuous multi-band photometric monitoring of the nuclear activity of comet 29P/Schwassmann-Wachmann 1 from 2008 to 2010. Our main aim has been to study the outburst mechanism on the basis of a follow-up of the…

We describe pre-perihelion optical observations of interstellar comet 3I/ATLAS taken during July - September 2025 using the Nordic Optical Telescope. Fixed aperture photometry of the comet is well described by a power law function of…

Earth and Planetary Astrophysics · Physics 2025-11-07 David Jewitt , Jane Luu

We present ALMA Band 6 observations of the CO(2-1), HCN(3-2), and HCO$^{+}$(3-2) lines in the nearby radio galaxy / brightest cluster galaxy (BCG) of NGC 1275 with the spatial resolution of $\sim20$ pc. In the previous observations, CO(2-1)…

Astrophysics of Galaxies · Physics 2019-10-09 H. Nagai , K. Onishi , N. Kawakatu , Y. Fujita , M. Kino , Y. Fukazawa , J. Lim , W. Forman , J. Vrtilek , K. Nakanishi , H. Noda , K. Asada , K. Wajima , Y. Ohyama , L. David

In December-2025, the NASA SPHEREx spacecraft re-observed ISO 3I/ATLAS post-perihelion, finding a much more active object compared to August-2025 SPHEREx pre-perihelion observations, with marked evidence for development into an cometary…

Multiple outbursts of a Jupiter-family comet, 15P/Finlay, occurred from late 2014 to early 2015. We conducted an observation of the comet after the first outburst and subsequently witnessed another outburst on 2015 January 15.6-15.7. The…

Aims. In this work, we present an extended study of the dust environment of a sample of short period comets and their dynamical history. With this aim, we characterized the dust tails when the comets are active, and we made a statistical…

We present observations of comet 67P/Churyumov-Gerasimenko acquired in support of the $Rosetta$ mission. We obtained usable data on 68 nights from 2014 September until 2016 May, with data acquired regularly whenever the comet was…

Earth and Planetary Astrophysics · Physics 2017-11-15 Matthew M. Knight , Colin Snodgrass , Jean-Baptiste Vincent , Blair Conn , Brian A. Skiff , David G. Schleicher , Tim Lister

Long period comet C/2021 A1 (Leonard) will approach Venus to within 0.029 au on 2021 December 18 and may subsequently graze the planet with its dust trail less than two days later. We observed C/2021 A1 with the Lowell Discovery Telescope…

Earth and Planetary Astrophysics · Physics 2021-10-19 Qicheng Zhang , Quanzhi Ye , Shreyas Vissapragada , Matthew M. Knight , Tony L. Farnham

The Atacama Large Millimeter/submillimeter Array Survey of Orion Planck Galactic Cold Clumps (ALMASOP) reveals complex nested morphological and kinematic features of molecular outflows through the CO (J = 2 - 1) and SiO (J = 5 - 4)…

Submillimetre and millimetre observations are important in probing the properties of the molecular gas and dust around obscured active galactic nuclei (AGNs) and their feedback. With very high-resolution (0."02x0."03 (2x3 pc)) ALMA 345 GHz…

We report photometric observations of comet 29P/Schwassmann-Wachmann 1 made on August 12, 2016 with the broadband B, V, R and I filters and the SOAR 4.1-meter telescope (Chile). We find the comet active at that time. Enhanced images…

Earth and Planetary Astrophysics · Physics 2020-12-22 E. Picazzio , I. V. Luk'yanyk , O. V. Ivanova , E. Zubko , O. Cavichia , G. Videen , S. M. Andrievsky

We present new observations of CO J=2-1 emission from the protoplanetary disk around TW Hya. Emission is detected out to 240 au (4") and found to exhibit azimuthal variations up to 20% beyond 180 au (3"), with the west side of the disk…

Earth and Planetary Astrophysics · Physics 2022-05-25 Richard Teague , Jaehan Bae , Myriam Benisty , Sean M. Andrews , Stefano Facchini , Jane Huang , David Wilner

The hot subdwarf HD 49798 has an X-ray emitting compact companion with a spin-period of 13.2 s and a dynamically measured mass of 1.28+/-0.05 M_sun, consistent with either a neutron star or a white dwarf. Using all the available XMM-Newton…

High Energy Astrophysical Phenomena · Physics 2016-03-23 Sandro Mereghetti , Fabio Pintore , Paolo Esposito , Nicola La Palombara , Andrea Tiengo , Gian Luca Israel , Luigi Stella

We observed comet C/2016 R2 (PANSTARRS) with the ARO 10-m SMT, and report the first detection of CO emission from this comet with amounts high enough to be the primary driver of activity. We obtained spectra and maps of the CO J=2-1…

Earth and Planetary Astrophysics · Physics 2018-07-18 Kacper Wierzchos , Maria Womack

We present the results of a global coma morphology campaign for comet C/2012 S1 (ISON), which was organized to involve both professional and amateur observers. In response to the campaign, many hundreds of images, from nearly two dozen…

Earth and Planetary Astrophysics · Physics 2015-12-23 Nalin H. Samarasinha , 48 co-authors

The CN coma structure of the EPOXI mission target, comet 103P/Hartley 2, was observed during twenty nights from September to December 2010. These CN images probe the rotational state of the comet's nucleus and provide a ground-based…

Earth and Planetary Astrophysics · Physics 2015-05-28 Nalin H. Samarasinha , Beatrice E. A. Mueller , Michael F. A'Hearn , Tony L. Farnham , Alan Gersch

The ASTEP (Antarctica Search for Transiting ExoPlanets) program was originally aimed at probing the quality of the Dome C, Antarctica for the discovery and characterization of exoplanets by photometry. In the first year of operation of the…