Search Publications

Objects of the Catalog of Orbits of Visual Binary Stars in Gaia DR2
DOI: 10.26087/INASAN.2019.3.1.056 Bibcode: 2019INASR...3..360C

Chulkov, D. A.

Cross-identification is made for the Catalog of Orbits of Visual Binary Stars and Gaia DR2. At least one component has been matched for 88% systems, for 15% identification is available for both stars. Systems with substantially different parallaxes of components are found, which are the candidates to be the optical pairs. It's shown that published…

2019 INASAN Science Reports
Gaia 2
ExoMars Flush Air Data System: Experimental and Numerical Investigation
DOI: 10.2514/1.A34185 Bibcode: 2019JSpRo..56..971S

Schleutker, Thorn; Gülhan, Ali; Hove, Bart Van +1 more

2019 Journal of Spacecraft and Rockets
ExoMars-16 2
Variability in high‑mass X‑ray binaries
DOI: 10.1002/asna.201913618 Bibcode: 2019AN....340..323F

Wilms, J.; Pottschmidt, K.; Grinberg, V. +5 more

Strongly magnetized, accreting neutron stars show periodic and aperiodic variability over a wide range of time scales. By obtaining spectral and timing information on these different time scales, we can have a closer look into the physics of accretion close to the neutron star and the properties of the accreted material. One of the most prominent …

2019 Astronomische Nachrichten
INTEGRAL 2
Search for Evolutionary Changes in the Periods of Cepheids: V532 Cyg
DOI: 10.1134/S1063773719100013 Bibcode: 2019AstL...45..677B

Berdnikov, L. N.

For the low-amplitude Cepheid V532 Cyg we have constructed an O - C diagram spanning a time interval of 121 years. The O - C diagram has the shape of a parabola, which has made it possible to determine for the first time the quadratic light elements and to calculate the rate of evolutionary decrease in the period, dP/dt = -0.248 (±0.067) s yr

2019 Astronomy Letters
INTEGRAL 2
Comparison of proper motions in declination for 387 Gaia DR2 and HIPPARCOS stars from ILS observations over many decades
DOI: 10.1051/0004-6361/201936541 Bibcode: 2019A&A...631A.145D

Taris, F.; Damljanović, G.

Context. The second solution of the Gaia catalog, which has been available since April 2018, plays an important role in the realization of the future Gaia reference frame. Since 1997, the reference frame has been materialized by the optical HIPPARCOS positions of about 120 000 stars. The HIPPARCOS has been compared with and linked to the Internati…

2019 Astronomy and Astrophysics
Gaia Hipparcos 2
Near- to mid-infrared spectroscopy of the heavily obscured AGN LEDA 1712304 with AKARI/IRC
DOI: 10.1051/0004-6361/201935483 Bibcode: 2019A&A...626A.130T

Oyabu, S.; Toba, Y.; Kaneda, H. +5 more

Context. Although heavily obscured active galactic nuclei (AGNs) have been found by many observational studies, the properties of the surrounding dust are poorly understood. Using AKARI/IRC spectroscopy, we discovered a new heavily obscured AGN in LEDA 1712304 which shows a deep spectral absorption feature due to silicate dust.
Aims: We study…

2019 Astronomy and Astrophysics
AKARI Herschel 2
A Photometric Study of the Contact Binary V384 Serpentis
Bibcode: 2019JAVSO..47...43M

Michaels, E. J.; Lanning, C. M.; Self, S. N.

In this paper we present the first photometric light curves in the Sloan g', r', and i' passbands for the contact binary V384 Ser. Photometric solutions were obtained using the Wilson-Devinney program which revealed the star to be a W-type system with a mass ratio of q = 2.65 and a f = 36% degree of contact. The less massive component was found to…

2019 Journal of the American Association of Variable Star Observers (JAAVSO)
Gaia 2
An XMM-Newton look at the strongly variable radio-weak BL Lac Fermi J1544-0639
DOI: 10.1051/0004-6361/201834662 Bibcode: 2019A&A...622A.116U

Pian, E.; Masetti, N.; Ubertini, P. +6 more

Context. Fermi J1544-0639/ASASSN-17gs/AT2017egv was identified as a gamma-ray/optical transient on May 15, 2017. Subsequent multiwavelength observations suggest that this source may belong to the new class of radio-weak BL Lacs.
Aims: We studied the X-ray spectral properties and short-term variability of Fermi J1544-0639 to constrain the X-ra…

2019 Astronomy and Astrophysics
XMM-Newton 2
Generalized Additive Modeling Combined With Multiple Collinear for ICME Velocity Forecasting
DOI: 10.1029/2018SW002135 Bibcode: 2019SpWea..17..567L

Ji, H. S.; Wang, M.; Lu, J. Y. +5 more

One of the main issues of space weather is the timely prediction of disturbed solar wind parameters at L1, especially caused by Coronal Mass Ejection (CME). Using the data from 170 front halo, flare-associated CMEs, and in-site solar wind data, an analysis of the Interplanetary Coronal Mass Ejection (ICME) peak velocity at L1 related to associated…

2019 Space Weather
SOHO 2
Ultraviolet HST Spectroscopy of Planck Cold Clumps
DOI: 10.3847/1538-4357/aaff5d Bibcode: 2019ApJ...872..140D

Meyer, David M.; Dirks, Cody

We report results of the first study utilizing the ultraviolet capabilities of the Hubble Space Telescope to investigate a sample of Planck Galactic Cold Clump (PGCC) sources. We have selected high-resolution spectra toward 25 stars that contain a multitude of interstellar absorption lines associated with the interstellar medium (ISM) gas within t…

2019 The Astrophysical Journal
Gaia eHST 2