中文
相关论文

相关论文: Discovery of Carbon Monoxide in Distant Comet C/20…

200 篇论文

Hyperactive comet activity typically becomes evident beyond the frost line (3 to 4 au) where it becomes too cold for water-ice to sublimate. If carbon monoxide (CO) and carbon dioxide (CO2) are the species that drive activity at…

地球与行星天体物理 · 物理学 2024-02-06 Dave G. Milewski , Joseph R. Masiero , Jana Pittichova , Emily A. Kramer , Amy K. Mainzer , James M. Bauer

We report on imaging and spectroscopic observations of comet C/2016~R2 (Pan-STARRS) obtained with the 0.8\,m and 2.7\,m telescopes of McDonald Observatory in November and December 2017 respectively. The comet was at a heliocentric distance…

地球与行星天体物理 · 物理学 2018-03-16 Anita L. Cochran , Adam J. McKay

We present analysis of observations of CO2 and OI emission in three comets to measure the CO2 abundance and evaluate the possibility of employing observations of OI emission in comets as a proxy for CO2. We obtained NIR imaging sensitive to…

Early observations of comet C/2016 R2 (PanSTARRS) have shown that the composition of this comet is very peculiar. We obtained high resolution spectra of the comet in February when it was at 2.8 au from the Sun. We used the UVES spectrograph…

地球与行星天体物理 · 物理学 2019-04-17 C. Opitom , D. Hutsemékers , E. Jehin , P. Rousselot , F. J. Pozuelos , J. Manfroid , Y. Moulane , M. Gillon , Z. Benkhaldoun

The N$_2$ and CO-rich and water-depleted comet C/2016 R2 (Pan-STARRS) (hereafter `C/2016 R2') is a unique comet for detailed spectroscopic analysis. We aim to explore the associated photochemistry of parent species, which produces different…

地球与行星天体物理 · 物理学 2020-03-25 S. Raghuram , D. Hutsemékers , C. Opitom , E. Jehin , A. Bhardwaj , J. Manfroid

(60558) 174P/Echeclus is an unusual object that belongs to a class of minor planets called Centaurs, which may be intermediate between Kuiper Belt Objects and Jupiter Family comets. It is sporadically active throughout its orbit at…

地球与行星天体物理 · 物理学 2017-04-28 Kacper Wierzchos , Maria Womack , Gal Sarid

We present a photometric and dynamical study of comet C/2010 U3 (Boattini), which was seen active in prediscovery data as early as 2005 November at a new inbound record heliocentric distance $r_{\rm H} = 25.8$ au. Two outburst events around…

地球与行星天体物理 · 物理学 2019-04-17 Man-To Hui , Davide Farnocchia , Marco Micheli

We present near-infrared spectroscopy of the NGC 5128 supernova SN 2016adj in the first 2 months following discovery. We report the detection of first overtone carbon monoxide emission at $\sim58.2$ d after discovery, one of the earliest…

We observed the new Long Period Comet C/2024 E1 (Wierzchos), inbound at 7 au from the Sun, using the NIRSpec integral field unit on JWST. The spectrum shows absorption features due to water ice in the coma and evidence for CO$_2$ driven…

The most extensive survey of carbon monoxide (CO) gas in the Taurus molecular cloud relied on $^{12}$CO and $^{13}$CO $J=1 \rightarrow 0$ emission only, distinguishing the region where $^{12}$CO is detected without $^{13}$CO (named mask 1…

星系天体物理 · 物理学 2023-08-02 Yan Duan , Di Li , Laurent Pagani , Paul F. Goldsmith , Tao-Chung Ching , Chen Wang , Jinjin Xie

(Abreviated) Comet C/2017 K2 PANSTARRS drew attention to its activity already at a time of its discovery in May 2017 when it was about 16 au from the Sun. This Oort spike comet will approach its perihelion in December 2022, and the question…

地球与行星天体物理 · 物理学 2018-11-15 Małgorzata Królikowska , Piotr A. Dybczyński

We aim to determine the production rates of several parent and product volatiles and the 12C/13C isotopic carbon ratio in the long-period comet C/2004 Q2 (Machholz), which is likely to originate from the Oort Cloud. The line emission from…

地球与行星天体物理 · 物理学 2012-09-04 M. de Val-Borro , P. Hartogh , C. Jarchow , M. Rengel , G. L. Villanueva , M. Küppers , N. Biver , D. Bockelée-Morvan , J. Crovisier

Recent observations of the long period comet C/2016 R2 (PanSTARRS) indicate an unusually high N2/CO abundance ratio, typically larger than 0.05, and at least 2-3 times higher than the one measured in 67P/Churyumov-Gerasimenko. Another…

The recent observations show that comet C/2016 R2 (Pan-Starrs) has a unique and peculiar composition when compared with several other comets observed at 2.8 au heliocentric distance. Assuming solar resonance fluorescence is the only…

地球与行星天体物理 · 物理学 2021-01-06 Susarla Raghuram , Anil Bhardwaj , Damien Hutsemékers , Cyrielle Opitom , Jean Manfroid , Emmanuel Jehin

Observations of the CO J(1-0) 115 GHz and J(2-1) 230 GHz lines in comet C/1995 O1 (Hale-Bopp) were performed with the IRAM Plateau de Bure interferometer on 11 March, 1997. The observations were conducted in both single-dish (ON-OFF) and…

地球与行星天体物理 · 物理学 2010-11-02 D. Bockelée-Morvan , F. Henry , N. Biver , J. Boissier , P. Colom , J. Crovisier , D. Despois , R. Moreno , J. Wink

Photometric and spectroscopic observations of five nearly parabolic comets with eccentricity larger than 0.99 at heliocentric distances greater than 4 AU were performed. No molecular emission was observed for any studied comet and the…

Comet C/2016 R2 PanSTARRS (hereafter C/2016 R2) presents an unusually high N2/CO abundance ratio, as well as a heavy depletion in H2O, making it the only known comet of its kind. Understanding its dynamical history is therefore of essential…

地球与行星天体物理 · 物理学 2022-11-09 S. E. Anderson , J. -M. Petit , B. Noyelles , O. Mousis , P. Rousselot

Pluto's icy surface has changed colour and its atmosphere has swelled since its last closest approach to the Sun in 1989. The thin atmosphere is produced by evaporating ices, and so can also change rapidly, and in particular carbon monoxide…

地球与行星天体物理 · 物理学 2015-05-27 J. S. Greaves , Ch. Helling , P. Friberg

To date, at least three comets -- 2I/Borisov, C/2016 R2 (PanSTARRS), and C/2009 P1 (Garradd) -- have been observed to have unusually high CO concentrations compared to water. We attempt to explain these observations by modeling the effect…

地球与行星天体物理 · 物理学 2021-05-26 Ellen M. Price , L. Ilsedore Cleeves , Dennis Bodewits , Karin I. Öberg

We report spectroscopic and imaging observations of rotational transitions of cold CO and SiO in the ejecta of SN1987A, the first such emission detected in a supernova remnant. In addition to line luminosities for the CO J=1-0, 2-1, 6-5,…