Search Publications

Photometric and Spectroscopic Studies of Superoutbursts of Three Dwarf Novae Independently Identified by the SVOM/GWAC System in 2018
DOI: 10.3847/1538-3881/ab5855 Bibcode: 2020AJ....159...35W

Zheng, W.; Filippenko, A. V.; Xu, Y. +27 more

We report our photometric and spectroscopic follow-up observations of the superoutbursts of three dwarf novae (DNe; GWAC 180415A, GWAC 181017A, and GWAC 181211A) identified independently by the Ground Wide-angle Cameras system, one of the ground-based instruments of the China-France SVOM mission. Based on a combination of our photometry and that t…

2020 The Astronomical Journal
Gaia 10
Identifying Multiple Populations in M71 Using CN
DOI: 10.3847/1538-3881/ab607e Bibcode: 2020AJ....159...50G

Vesperini, Enrico; Gerber, Jeffrey M.; Friel, Eileen D.

We have observed the CN features at ∼3800 and 4120 Å as well as the CH band at ∼4300 Å for 145 evolved stars in the Galactic globular cluster M71 using the multi-object spectrograph, Hydra, on the Wisconsin-Indiana-Yale-NOAO-3.5 m telescope. We use these measurements to create two δCN indices finding that both distributions are best fit by two pop…

2020 The Astronomical Journal
eHST 10
Study of Star Clusters in the M83 Galaxy with a Convolutional Neural Network
DOI: 10.3847/1538-3881/abbf53 Bibcode: 2020AJ....160..264B

Bialopetravičius, Jonas; Narbutis, Donatas

We present a study of evolutionary and structural parameters of star cluster candidates in the spiral galaxy M83. For this we use a convolutional neural network trained on mock clusters and capable of fast identification and localization of star clusters, as well as inference of their parameters from multiband images. We use this pipeline to detec…

2020 The Astronomical Journal
eHST 10
Optical Linear Polarization toward the Open Star Cluster Casado Alessi 1
DOI: 10.3847/1538-3881/ab6608 Bibcode: 2020AJ....159...99S

Yadav, R. K. S.; Medhi, Biman J.; Pandey, Jeewan C. +1 more

We present B-, V-, R-, and I-band linear polarimetric observations of 73 stars in the direction of open star cluster Casado Alessi 1 (hereafter Alessi 1). We aim to use polarimetry as a tool to investigate the properties and distribution of dust grains toward the direction of the cluster. The polarimetric observations were carried out using the AR…

2020 The Astronomical Journal
Gaia 10
Spectroscopic Studies of 30 Short-period Cataclysmic Variable Stars and Remarks on the Evolution and Population of Similar Objects
DOI: 10.3847/1538-3881/ab911c Bibcode: 2020AJ....160....6T

Thorstensen, John R.

We present spectroscopy and orbital periods Porb for 30 apparently nonmagnetic cataclysmic binaries with periods below ∼3 hr, nearly all of which are dwarf novae, mostly of the SU Ursae Majoris subclass. We then turn to the evidence supporting the prediction that short-period dwarf novae evolve toward longer periods after passing throug…

2020 The Astronomical Journal
Gaia 10
A Random Forest Approach to Identifying Young Stellar Object Candidates in the Lupus Star-forming Region
DOI: 10.3847/1538-3881/ab72ac Bibcode: 2020AJ....159..200M

Melton, Elizabeth

The identification and characterization of stellar members within a star-forming region are critical to many aspects of star formation, including formalization of the initial mass function, circumstellar disk evolution, and star formation history. Previous surveys of the Lupus star-forming region have identified members through infrared excess and…

2020 The Astronomical Journal
Gaia 10
Probing UV-sensitive Pathways for CN and HCN Formation in Protoplanetary Disks with the Hubble Space Telescope
DOI: 10.3847/1538-3881/ab789a Bibcode: 2020AJ....159..168A

France, Kevin; Hoadley, Keri; Manara, Carlo F. +6 more

The UV radiation field is a critical regulator of gas-phase chemistry in surface layers of disks around young stars. In an effort to understand the relationship between photocatalyzing UV radiation fields and gas emission observed at infrared and submillimeter wavelengths, we present an analysis of new and archival Hubble Space Telescope (HST), Sp…

2020 The Astronomical Journal
eHST 10
Mathematical Underpinnings of the Multiwavelength Structure of the Tip of the Red Giant Branch
DOI: 10.3847/1538-3881/abab9a Bibcode: 2020AJ....160..170M

Madore, Barry F.; Freedman, Wendy L.

We consider the application of the tip of the red giant branch (TRGB) in the optical and in the near-infrared for the determination of distances to nearby galaxies. We analyze ACS VI (F555W and F814W) data and self-consistently cross-calibrate WFC3-IR JH (F110W and F120W) data using an absolute magnitude calibration of MI = -4.05 mag as…

2020 The Astronomical Journal
eHST 9
New Candidates for Planetary-mass Brown Dwarfs in IC 348
DOI: 10.3847/1538-3881/ab96bb Bibcode: 2020AJ....160...57L

Luhman, K. L.; Hapich, C. J.

We have used infrared images obtained with the Wide Field Camera 3 on board the Hubble Space Telescope to search for planetary-mass brown dwarfs in the star-forming cluster IC 348. In those images, we have identified 12 objects that have colors indicative of spectral types later than M8, corresponding to masses of ≲30 MJup at the age of…

2020 The Astronomical Journal
eHST 9
Proper-motion Membership Tests for Four Planetary Nebulae in Galactic Globular Clusters
DOI: 10.3847/1538-3881/ab8f9e Bibcode: 2020AJ....159..276B

Bond, Howard E.; Sahu, Kailash C.; Bellini, Andrea

Four planetary nebulae (PNe) are considered to be probable or possible members of Galactic globular clusters (GCs). These are Ps 1 = K648 in M15, GJJC 1 = IRAS 18333-2357 in M22, JaFu 1 in Palomar 6, and JaFu 2 in NGC 6441. In addition to lying close to the host GCs on the sky, these PNe have radial velocities that are consistent, within the error…

2020 The Astronomical Journal
Gaia eHST 9