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EPIC 216747137 is a new HW~Virginis system discovered by the Kepler spacecraft during its K2 "second life". Like the other HW Vir systems, EPIC 216747137 is a post-common-envelope eclipsing binary consisting of a hot subluminous star and a…

Solar and Stellar Astrophysics · Physics 2020-11-04 R. Silvotti , V. Schaffenroth , U. Heber , R. H. Østensen , J. H. Telting , J. Vos , D. Kilkenny , L. Mancini , S. Ciceri , A. Irrgang , H. Drechsel

We present optical and near-IR spectroscopy of a z=2.38 hyperluminous IR galaxy, covering the restframe wavelength range from 1000-5000A. It appears to comprise two components separated by less than 1" on the sky (<8kpc); one component (B)…

We report the detection of large-amplitude, rapid radial velocity (RV) variations and line-splitting in high-resolution Keck/NIRSPEC spectra of the M9 dwarf LP 413-53. We attribute these features to binary motion. Analyzing data spanning 15…

Solar and Stellar Astrophysics · Physics 2023-03-08 Chih-Chun Hsu , Adam J. Burgasser , Christopher A. Theissen

We present the first observations of hydrogen line emission detected around the B-type star HD 46487, a well-studied star in the CoRoT field of view. The emission is only evident in the H$\alpha$ line, for which the observed violet-red peak…

Solar and Stellar Astrophysics · Physics 2017-05-26 David G. Whelan , R. David Baker

We present multi-epoch high-resolution optical spectroscopy ($R \simeq 80{,}000$) of the emission-line object NaSt1 to test its proposed binary nature, along with long-term multiband photometry, mid-infrared spectroscopy, and spatially…

We present Chandra X-ray images for the interacting galaxy pair NGC 7714/5. In addition to the unresolved starburst nucleus, a variable point source with L(X) ~ 10^40 erg/s was detected 1.5" (270 pc) northwest of the nucleus, coincident…

Astrophysics · Physics 2009-11-10 Beverly J. Smith , Curtis Struck , Michael A. Nowak

HD50138 is a Herbig B[e] star with a circumstellar disc detected at IR and mm wavelength. Its brightness makes it a good candidate for NIR interferometry observations. We aim to resolve, spatially and spectrally, the continuum and hydrogen…

Solar and Stellar Astrophysics · Physics 2018-06-27 M. Koutoulaki , R. Garcia Lopez , A. Natta , A. Caratti o Garatti , D. Coffey , J. Sanchez-Bermudez , T. P. Ray

We present high angular resolution, high-sensitivity Very Large Array observations at 3.6 cm of the Herbig Ae star AB Aur. This star is of interest since its circumstellar disk exhibits characteristics that have been attributed to the…

Astrophysics · Physics 2007-05-23 Luis F. Rodriguez , Luis Zapata , Paul T. P. Ho

Using one archival high dispersion high quality spectrum of HR8844 (A0V) obtained with the echelle spectrograph SOPHIE at Observatoire de Haute Provence, we show that this star is not a superficially normal A0V star as hitherto thought. The…

Solar and Stellar Astrophysics · Physics 2016-09-19 R. Monier , M. Gebran , F. Royer

We present new Very Large Array HI spectral line, archival Sloan Digital Sky Survey, and archival Spitzer Space Telescope imaging of eight star-forming blue compact dwarf galaxies that were selected to be optically compact (optical radii…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Hans P. Most , John M. Cannon , John J. Salzer , Jessica J. Rosenberg , Eric Engstrom , Palmer Fliss

We report evidence for a planetary companion around the nearby young star HD 70573. The star is a G type dwarf located at a distance of 46 pc with age estimation between 20 and 300 Myrs. We carried out spectroscopic observations of this…

Astrophysics · Physics 2015-05-13 J. Setiawan , P. Weise , Th. Henning , R. Launhardt , A. Müller , J. Rodmann

High-resolution spectroscopy and speckle interferometry reveal the young star HD 86588 as a quadruple system with a 3-tier hierarchy. The 0.3" resolved binary A,B with an estimated period around 300 years contains the 8-year pair Aa,Abc…

Solar and Stellar Astrophysics · Physics 2018-08-29 Andrei Tokovinin , Hank Corbett , Octavi Fors , Ward Howard , Nicholas M. Law , Maxwell Moe , Frederick M. Walter

We present 18 years of OGLE photometry together with spectra obtained over 12 years, revealing that the early Oe star AzV 493 shows strong photometric (Delta I < 1.2 mag) and spectroscopic variability with a dominant, 14.6-year pattern and…

We analyse the spectroscopic and photometric variability of the Oe star HD 60848 over the last twenty five years. The spectra reveal recurrent, but irregular cycles of increased circumstellar emission lines. These cycles are highly…

Solar and Stellar Astrophysics · Physics 2020-12-09 Gregor Rauw , Yael Naze , Fran Campos , Joan Guarro Flo , Umberto Sollecchia

The analysis of the available TESS light curves of $\alpha$ Sex (HD 87887) reveals low-frequency pulsations with a period of about 9.1 hours in this spectroscopic A0 III standard star. The IUE observations in December 1992 reveal large flux…

Solar and Stellar Astrophysics · Physics 2023-08-02 Richard Monier , Dominic M. Bowman , Yveline Lebreton , Morgan Deal

We present ground-based optical and near infrared photometric observations and Hubble Space Telescope COS spectroscopic observations of the old nova V842 Cen (Nova Cen 1986). Analysis of the optical light curves reveals a peak at 56.5 +/-…

Solar and Stellar Astrophysics · Physics 2015-06-16 Edward M. Sion , Paula Szkody , Anjum Mukadam , Brian Warner , Patrick Woudt , Frederic Walter , Arne Henden , Patrick Godon

V347 Aurigae is associated with the small dark cloud L1438 and appears to be an isolated pre-main sequence star located at distance $d\approx$200 pc. Multi-epoch, archival photometry reveals periodic brightness variations with amplitude…

Solar and Stellar Astrophysics · Physics 2020-12-02 S. E. Dahm , L. A. Hillenbrand

We report extensive new photometry and spectroscopy of the highly variable young stellar object PTF 10nvg including optical and near-infrared time series data as well as mid-infrared and millimeter data. Following the previously reported…

We present ultraviolet (UV) spectroscopy of the 17 Myr, G0V star, HIP 67522. The UV spectrum is characterized by strong chromospheric and transition region emission lines. There was moderate spectral variability during the observations…

We present a study of low- and high-resolution ultraviolet, high-resolution optical CAT/CES spectra and ultraviolet, optical and infrared photometry of the peculiar supergiant HD101584. From the photometry we learn that the ultraviolet and…

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