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In the last decades Near-Earth Objects (NEOs) have become very important targets to study, since they can give us clues to the formation, evolution and composition of the Solar System. In addition, they may represent either a threat to…

Earth and Planetary Astrophysics · Physics 2014-09-24 S. Ieva , E. Dotto , D. Perna , M. A. Barucci , F. Bernardi , S. Fornasier , F. De Luise , E. Perozzi , A. Rossi , J. R. Brucato

Cometary activity is a manifestation of sublimation-driven processes at the surface of nuclei. However, cometary outbursts may arise from other processes that are not necessarily driven by volatiles. In order to fully understand nuclear…

We present a measurement of the lifetime of ground state atomic carbon, C(^3P), against ionization processes in interplanetary space and compare it to the lifetime expected from the dominant physical processes likely to occur in this…

Earth and Planetary Astrophysics · Physics 2015-05-20 Jeffrey P. Morgenthaler , Walter M. Harris , Michael R. Combi , Paul D. Feldman , Harold A. Weaver

Main belt comets (MBCs) are a peculiar class of volatile-containing objects with comet-like morphology and asteroid-like orbits. However, MBCs are challenging targets to study remotely due to their small sizes and the relatively large…

Earth and Planetary Astrophysics · Physics 2019-11-20 B. Yang , E. Jehin , F. J. Pozuelos , Y. Moulane , Y. Shinnaka , C. Opitom , H. H. Hsieh , D. Hutsemékers , J. Manfroid

We study the sensitivity of nEXO to solar neutrino charged-current interactions, $\nu_e + ^{136}$Xe$\rightarrow ^{136}$Cs$^* + e^-$, as well as analogous interactions predicted by models of fermionic dark matter. Due to the recently…

Nuclear Experiment · Physics 2025-07-01 G. Richardson , B. G. Lenardo , D. Gallacher , R. Saldanha , P. Acharya , S. Al Kharusi , A. Amy , E. Angelico , A. Anker , I. J. Arnquist , A. Atencio , J. Bane , V. Belov , E. P. Bernard , T. Bhatta , A. Bolotnikov , J. Breslin , P. A. Breur , J. P. Brodsky , S. Bron , E. Brown , T. Brunner , B. Burnell , E. Caden , G. F. Cao , L. Q. Cao , D. Cesmecioglu , D. Chernyak , M. Chiu , R. Collister , T. Daniels , L. Darroch , R. DeVoe , M. L. di Vacri , M. J. Dolinski , B. Eckert , M. Elbeltagi , A. Emara , N. Fatemighomi , W. Fairbank , B. T. Foust , N. Gallice , G. Giacomini , W. Gillis , A. Gorham , R. Gornea , K. Gracequist , G. Gratta , C. A. Hardy , S. C. Hedges , M. Heffner , E. Hein , J. D. Holt , A. Iverson , P. Kachru , A. Karelin , D. Keblbeck , I. Kotov , A. Kuchenkov , K. S. Kumar , A. Larson , M. B. Latif , S. Lavoie , K. G. Leach , A. Lennarz , D. S. Leonard , K. K. H. Leung , H. Lewis , G. Li , X. Li , Z. Li , C. Licciardi , R. Lindsay , R. MacLellan , S. Majidi , C. Malbrunot , M. Marquis , J. Masbou , M. Medina-Peregrina , S. Mngonyama , B. Mong , D. C. Moore , X. E. Ngwadla , K. Ni , A. Nolan , S. C. Nowicki , J. C. Nzobadila Ondze , A. Odian , J. L. Orrell , G. S. Ortega , L. Pagani , H. Peltz Smalley , A. Peña Perez , A. Piepke , A. Pocar , V. Radeka , R. Rai , H. Rasiwala , D. Ray , S. Rescia , F. Retière , V. Riot , N. Rocco , R. Ross , P. C. Rowson , S. Sangiorgio , S. Sekula , T. Shetty , L. Si , J. Soderstrom , F. Spadoni , V. Stekhanov , X. L. Sun , S. Thibado , T. Totev , S. Triambak , R. H. M. Tsang , O. A. Tyuka , T. Vallivilayil John , E. van Bruggen , M. Vidal , S. Viel , J. Vuilleumier , M. Walent , H. Wang , Q. D. Wang , M. P. Watts , W. Wei , M. Wehrfritz , L. J. Wen , U. Wichoski , S. Wilde , M. Worcester , X. M. Wu , H. Xu , H. B. Yang , L. Yang , O. Zeldovich

The cosmic X-ray background (CXB) is dominated by the obscured and unobscured coronal light of active galactic nuclei (AGN). At energies below 10 keV, the CXB can be well explained by models taking into account the known AGN and the…

High Energy Astrophysical Phenomena · Physics 2025-02-03 Isaiah S. Cox , Núria Torres-Albà , Stefano Marchesi , Peter Boorman , Xiurui Zhao , Ross Silver , Marco Ajello , Indrani Pal

The growth of active galactic nuclei (AGN) occurs under some form of obscuration in a large fraction of the population. The difficulty in constraining this population leads to high uncertainties in cosmic X-ray background and galaxy…

Astrophysics of Galaxies · Physics 2024-01-05 Claire Greenwell , Poshak Gandhi , Daniel Stern , George Lansbury , Vincenzo Mainieri , Peter Boorman , Yoshiki Toba

We present the results of ROSAT and XMM-Newton observations of the recurrent ultraluminous X-ray source (ULX) NGC 253 ULX1. This transient is one of the few ULXs that was detected during several outbursts. The luminosity reached 1.4 10^39…

Astrophysics · Physics 2009-11-11 M. Bauer , W. Pietsch

We present our results for comet (ISON). Our results were obtained with amateur telescopes observing from the ground, before and after the comet had passed conjunction with the Sun in August 2013. We measured a mean radius of 830 +- 245 m,…

Solar and Stellar Astrophysics · Physics 2014-05-14 Toni Scarmato

We present a detailed spectral analysis of the black hole candidate MAXI J1836-194. The source was caught in the intermediate state during its 2011 outburst by Suzaku and RXTE. We jointly fit the X-ray data from these two missions using the…

High Energy Astrophysical Phenomena · Physics 2020-02-19 Yanting Dong , Javier A. García , Zhu Liu , Xueshan Zhao , Xueying Zheng , Lijun Gou

Context. Centaurs go around the Sun between the orbits of Jupiter and Neptune. Only a fraction of the known centaurs have been found to display comet-like features. Comet 29P/Schwassmann-Wachmann 1 is the most remarkable active centaur. It…

Earth and Planetary Astrophysics · Physics 2021-05-14 C. de la Fuente Marcos , R. de la Fuente Marcos , J. Licandro , M. Serra-Ricart , S. Martino , J. de Leon , F. Chaudry , M. R. Alarcon

We present observations showing in-bound long-period comet C/2017 K2 (PANSTARRS) to be active at record heliocentric distance. Nucleus temperatures are too low (60 K to 70 K) either for water ice to sublimate or for amorphous ice to…

Earth and Planetary Astrophysics · Physics 2017-10-04 David Jewitt , Man-To Hui , Max Mutchler , Harold Weaver , Jing Li , Jessic Agarwal

The recent close approach of comet C/2020 F3 (NEOWISE) allowed us to study the morphology of its inner coma. From the measurement of the dust ejection velocityon spiral structures expanding around the nucleus, we estimated a mean…

Earth and Planetary Astrophysics · Physics 2021-09-07 F. Manzini , V. Oldani , P. Ochner , E. Barbotin , L. R. Bedin , R. Behrend , G. Fardelli

We present independent polarimetric observations of the interstellar object 3I/ATLAS, including the first near-infrared polarimetric measurements. Using imaging polarimeters, we measured the degree of linear polarization from the visible RC…

We observed dynamically new sungrazing comet ISON (C/2012 S1) extensively at Lowell Observatory throughout 2013 in order to characterize its behavior prior to perihelion. ISON had "typical" abundances for an Oort Cloud comet. Its dust…

Earth and Planetary Astrophysics · Physics 2015-06-23 Matthew M. Knight , David G. Schleicher

Ultralight dark matter candidates, such as axions and dark photons, are leading dark matter candidates. They may couple feebly to photons, sourcing oscillating electromagnetic signals in the Earth's conducting cavity formed between the…

High Energy Physics - Phenomenology · Physics 2025-12-08 Ariel Arza , Yuanlin Gong , Jun Guo , Xiaofei Huang , Jing Shu , Hongliang Tian , Wenyu Wang , Kai Wei , Lei Wu , Mingming Xia , Jin Min Yang , Qiang Yuan , Yang Zhang , Yi Zhang , Bin Zhu

We report an XMM-Newton observation of the Low mass X-ray Binary (LMXB) and black hole candidate 4U1755-33. This source had been a bright persistent source for at least 25 yrs, but in 1995 entered an extended quiescent phase. 4U1755-33 was…

Astrophysics · Physics 2009-11-07 L. Angelini , N. E. White

Long-period comets are planetesimal remnants constraining the environment and volatiles of the protoplanetary disc. We report the discovery of hyperbolic long-period comet C/2022 E3 (ZTF), which has a perihelion $\sim$1.11 au, an…

We report on the identification of a new possible Isolated Neutron Star candidate in archival ROSAT observations. The source 1RXS J214303.7+065419, listed in the ROSAT Bright Survey as RBS 1774, is very soft, exhibits a thermal spectrum…

Astrophysics · Physics 2009-11-07 L. Zampieri , S. Campana , R. Turolla , M. Chieregato , R. Falomo , D. Fugazza , A. Moretti , A. Treves