Search Publications

Integrated approach to the PDR/H II complex by the application of carbon radio recombination lines in the millimetre range and fine-structure lines of C II and O I
DOI: 10.1093/mnras/stz3221 Bibcode: 2020MNRAS.492.1049S

Siddiqui, S. A.; Khan, Shafiqullah; Qaiyum, A.

We have performed self-consistent calculations to estimate the physical parameters of photodissociation regions (PDRs) associated with objects, namely, NGC 2024, Orion A and W3, using far-infrared continuum emission, fine-structure lines of C II and O I, and radio recombination lines of carbon. Typically, PDRs separate H II regions from the molecu…

2020 Monthly Notices of the Royal Astronomical Society
ISO 1
Coupling Mars Ground and Orbital Views: Generate Viewsheds of Mastcam Images From the Curiosity Rover, Using ArcGIS® and Public Datasets
DOI: 10.1029/2020EA001247 Bibcode: 2020E&SS....701247N

Stein, N.; Nachon, M.; Borges, S. +3 more

The Mastcam (Mast Camera) instrument onboard the NASA Curiosity rover provides an exclusive view of Mars: High-resolution color images from Mastcam allow users to study Gale crater's geologic terrains along Curiosity's path. These ground observations complement the spatially broader views of Gale crater provided by spacecrafts from orbit. However,…

2020 Earth and Space Science
MEx 1
Serendipitous Discovery of a Physical Binary Quasar at z = 1.76
DOI: 10.3847/1538-3881/ab6e67 Bibcode: 2020AJ....159..122A

Geier, S.; Fynbo, J. P. U.; Heintz, K. E. +7 more

Binary quasars are extremely rare objects, used to investigate clustering on very small scales at different redshifts. The cases where the two quasar components are gravitationally bound, known as physical binary quasars, can also exhibit enhanced astrophysical activity and therefore are of particular scientific interest. Here we present the seren…

2020 The Astronomical Journal
Gaia 1
Investigating the Physical Conditions in Extended System Hosting Mid-infrared Bubble N14
DOI: 10.3847/1538-4357/ab964c Bibcode: 2020ApJ...898...41D

Dewangan, L. K.; Ojha, D. K.; Baug, T. +1 more

To observationally explore physical processes, we present a multiwavelength study of a wide-scale environment toward l = 13°7-14°9 containing a mid-infrared bubble N14. The analysis of 12CO, 13CO, and C18O gas at [31.6, 46] km s-1 reveals an extended physical system (extension ∼59 pc × 29 pc), which host…

2020 The Astrophysical Journal
Herschel 1
Using the Modified Lognormal Power-law Distribution to Model the Mass Function of NGC 1711
DOI: 10.3847/1538-4357/ab88a6 Bibcode: 2020ApJ...895...66M

Basu, Shantanu; Madaan, Deepakshi; Lianou, Sophia

A determination of the mass function (MF) of stellar clusters can be quite dependent on the range of measured masses, the fitting technique, and the analytic function that is being fit to the data. Here, we use Hubble Space Telescope/WFPC2 data of NGC 1711, a stellar cluster in the Large Magellanic Cloud, as a test case to explore a range of possi…

2020 The Astrophysical Journal
eHST 1
A search for supernova light echoes in NGC 6946 with SITELLE
DOI: 10.1093/mnras/staa2006 Bibcode: 2020MNRAS.497.3297R

Welch, D. L.; Radica, M. C.; Rousseau-Nepton, L.

We present the analysis of 4 h of spectroscopic observations of NGC 6946 with the SITELLE Imaging Fourier Transform Spectrometer on the Canada-France-Hawaii Telescope, acquired to search for supernova light echoes from its 10 modern supernovae. We develop a novel spectroscopic search method: identifying negatively sloped continua in the narrow-ban…

2020 Monthly Notices of the Royal Astronomical Society
eHST 1
A Photometric Study of the Contact Binary GR Piscium
Bibcode: 2020JAVSO..48..193M

Michaels, E. J.

High-quality CCD photometric light curves of the eclipsing binary GR Psc are presented. The new multicolor light curves display total eclipses which were analyzed using the Wilson-Devinney program. The light curve solution describes the system as a contact configuration with a mass ratio of M2 / M1 = 0.431, a fill-out of f = 47%, and a small tempe…

2020 Journal of the American Association of Variable Star Observers (JAAVSO)
Gaia 1
Pixel-based Spectral Characterization of Mid-infrared Si Array Detectors for Astronomical Observations in Space
DOI: 10.1088/1538-3873/ab8aa8 Bibcode: 2020PASP..132g4502T

Kaneda, Hidehiro; Ishihara, Daisuke; Wada, Takehiko +2 more

Mid-infrared (IR) array detectors have been used for astronomical observations in space. However, the uniformities of their spectral response curves have not been investigated in detail, the understanding of which is important for spectroscopic observations using large array formats. We characterize the spectral responses of all the pixels in IR a…

2020 Publications of the Astronomical Society of the Pacific
AKARI 1
Multiwavelength Analysis of the Kinematics of a Long Duration Flare-CME Event on 27 January 2012
DOI: 10.1007/s11207-020-01693-1 Bibcode: 2020SoPh..295..121S

Shanmugaraju, A.; Suresh, K.; Selvarani, G. +1 more

We present a detailed analysis of a long-duration flare associated with a coronal mass ejection (CME) event that occurred on 27 January 2012 in the active region (AR) 11402. We analyze the kinematics of the CME and the close relationship between the flare, radio burst, and CME. We used STEREO (Solar Terrestrial Relations Observatory)/EUVI A (Extre…

2020 Solar Physics
SOHO 1
Multi-wavelength study in the region of IRAS 16571-4029 and 16575-4023 sources
DOI: 10.1016/j.newast.2020.101384 Bibcode: 2020NewA...7901384B

Baume, G.; Borissova, J.; Ramirez Alegria, S. +2 more

We studied the stellar populations and their associated interstellar medium structures located in the region of IRAS 16571-4029 and 16575-4023 sources, aiming to evaluate their distance and their main physical parameters. We focused our attention on the embedded cluster DBS 113 and its associated HII region RCW 116B.

For the study, optical im…

2020 New Astronomy
Gaia Herschel 1