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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004987naa a2200949 4500
001oai:DiVA.org:su-183956
003SwePub
008200828s2020 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1839562 URI
024a https://doi.org/10.3847/1538-3881/ab93052 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Bolin, Bryce T.4 aut
2451 0a Characterization of the Nucleus, Morphology, and Activity of Interstellar Comet 2I/Borisov by Optical and Near-infrared GROWTH, Apache Point, IRTF, ZTF, and Keck Observations
264 c 2020-06-17
264 1b American Astronomical Society,c 2020
338 a print2 rdacarrier
520 a We present visible and near-infrared (NIR) photometric and spectroscopic observations of interstellar object (ISO) 2I/Borisov taken from 2019 September 10 to 2019 December 20 using the GROWTH, the Apache Point Observatory Astrophysical Research Consortium 3.5 m, and the NASA Infrared Telescope Facility 3.0 m combined with pre- and postdiscovery observations of 2I obtained by the Zwicky Transient Facility from 2019 March 17 to 2019 May 5. Comparison with imaging of distant solar system comets shows an object very similar to mildly active solar system comets with an outgassing rate of similar to 10(27)mol s(-1). The photometry, taken in filters spanning the visible and NIR range, shows a gradual brightening trend of similar to 0.03 mag day(-1)since 2019 September 10 UTC for a reddish object becoming neutral in the NIR. The light curve from recent and prediscovery data reveals a brightness trend suggesting the recent onset of significant H2O sublimation with the comet being active with super volatiles such as CO at heliocentric distances >6 au consistent with its extended morphology. Using the advanced capability to significantly reduce the scattered light from the coma enabled by high-resolution NIR images from Keck adaptive optics taken on 2019 October 4, we estimate a diameter for 2I's nucleus of less than or similar to 1.4 km. We use the size estimates of 1I/'Oumuamua and 2I/Borisov to roughly estimate the slope of the ISO size distribution, resulting in a slope of similar to 3.4 1.2, similar to solar system comets and bodies produced from collisional equilibrium.
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
653 a Comets
653 a Minor planets
700a Lisse, Carey M.4 aut
700a Kasliwal, Mansi M.4 aut
700a Quimby, Robert4 aut
700a Tan, Hanjie4 aut
700a Copperwheat, Chris M.4 aut
700a Lin, Zhong-Yi4 aut
700a Morbidelli, Alessandro4 aut
700a Abe, Lyu4 aut
700a Bendjoya, Philippe4 aut
700a Burdge, Kevin B.4 aut
700a Coughlin, Michael4 aut
700a Fremling, Christoffer4 aut
700a Itoh, Ryosuke4 aut
700a Koss, Michael4 aut
700a Masci, Frank J.4 aut
700a Maeno, Syota4 aut
700a Mamajek, Eric E.4 aut
700a Marocco, Federico4 aut
700a Murata, Katsuhiro4 aut
700a Rivet, Jean-Pierre4 aut
700a Sitko, Michael L.4 aut
700a Stern, Daniel4 aut
700a Vernet, David4 aut
700a Walters, Richard4 aut
700a Yan, Lin4 aut
700a Andreoni, Igor4 aut
700a Bhalerao, Varun4 aut
700a Bodewits, Dennis4 aut
700a De, Kishalay4 aut
700a Deshmukh, Kunal P.4 aut
700a Bellm, Eric C.4 aut
700a Blagorodnova, Nadejda4 aut
700a Buzasi, Derek4 aut
700a Cenko, S. Bradley4 aut
700a Chang, Chan-Kao4 aut
700a Chojnowski, Drew4 aut
700a Dekany, Richard4 aut
700a Duev, Dmitry A.4 aut
700a Graham, Matthew4 aut
700a Juric, Mario4 aut
700a Kulkarni, Shrinivas R.4 aut
700a Kupfer, Thomas4 aut
700a Mahabal, Ashish4 aut
700a Neill, James D.4 aut
700a Ngeow, Chow-Choong4 aut
700a Penprase, Bryan4 aut
700a Riddle, Reed4 aut
700a Rodriguez, Hector4 aut
700a Smith, Roger M.4 aut
700a Rosnet, Philippe4 aut
700a Sollerman, Jesperu Stockholms universitet,Institutionen för astronomi4 aut0 (Swepub:su)solle
700a Soumagnac, Maayane T.4 aut
710a Stockholms universitetb Institutionen för astronomi4 org
773t Astronomical Journald : American Astronomical Societyg 160:1q 160:1x 0004-6256x 1538-3881
856u https://authors.library.caltech.edu/99959/2/Bolin_2020_AJ_160_26.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-183956
8564 8u https://doi.org/10.3847/1538-3881/ab9305

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