Search Publications

The nature of the solar wind electron temperature and electron heat flux. II. Case of a spiral interplanetary magnetic field
DOI: 10.1051/0004-6361/202244129 Bibcode: 2023A&A...677A.132H

Salem, Chadi S.; Pulupa, Marc; Hubert, Daniel


Aims: We aim to analyze the solutions of the solar wind electron energy equation in a spherical expansion with a spiral interplanetary magnetic field (IMF), a radial power law of the electron heat flux with a constant index α, and a constant or a smooth increase of the solar wind speed.
Methods: Generic analytical electron temperature pr…

2023 Astronomy and Astrophysics
Ulysses 0
TÜBİTAK TUG T60 ve İstanbul Üniversitesi İST60'ın GAIA Gözlemlerindeki Bazı Kataklismik Değişen Adaylarının Işık Eğrileri
DOI: 10.55064/tjaa.1200196 Bibcode: 2023TJAA....4S.392E

Esenoğlu, Hasan H.; Hamed, Gamal; Dağ, Meryem Kübra

Gaia uyarıları içerisinde 5 adet kataklismik değişen (CV) adayı (Gaia16ahl, 16bnz, 14adn, 16awq ve 21bpe) küçük açıklıklı robotik teleskoplarla (büyük olanlarla da koordineli şekilde) B, V, R süzgeçlerinde ve filtresiz olarak gözlenmiştir. Adayların tanımlamaları şöyledir: 16ahl-CV, 16bnz-bilinmeyen, 14adn-bilinmeyen, 16awq-bilinmeyen ve 21bpe-nov…

2023 Turkish Journal of Astronomy and Astrophysics
Gaia 0
SITCoM: SiRGraF Integrated Tool for Coronal dynaMics
DOI: 10.3389/fspas.2023.1227872 Bibcode: 2023FrASS..1027872U

Patel, Ritesh; Udhwani, Purvi; Shrivastav, Arpit Kumar

SiRGraF Integrated Tool for Coronal dynaMics (SITCoM) is based on the Simple Radial Gradient Filter used to filter the radial gradient in the white-light coronagraph images and bring out dynamic structures. SITCoM has been developed in Python and integrated with SunPy and can be installed by users with the command pip install sitcom. This enables …

2023 Frontiers in Astronomy and Space Sciences
SOHO 0
ORIGO: A mission concept to challenge planetesimal formation theories
DOI: 10.3389/frspt.2022.1054360 Bibcode: 2023FrST....354360M

Mottola, Stefano; Vincent, Jean-Baptiste; Thomas, Nicolas +12 more

Comets are generally considered among the most pristine objects in our Solar System. There have thus been significant efforts to understand these bodies. During the past decades, we have seen significant progress in our theoretical understanding of planetesimal/cometesimals (the precursors of comets) formation. Recent space missions—such as ESA's …

2023 Frontiers in Space Technologies
Rosetta 0
Noise effect of test mass surface roughness in spaceborne gravitational wave detectors
DOI: 10.1103/PhysRevD.108.042001 Bibcode: 2023PhRvD.108d2001Y

Wang, Shun; Yan, Hao; Miao, Haixing +2 more

The spaceborne gravitational wave detection mission has a demanding requirement for the precision of displacement sensing, which is conducted by the interaction between the laser field and test mass. However, due to the roughness of the reflecting surface of the test mass, the displacement measurement along the sensitive axis suffers a coupling er…

2023 Physical Review D
LISAPathfinder 0
ASASSN-18aan revisited
DOI: 10.5817/OEJV2023-0236 Bibcode: 2023OEJV..236....1N

Nelson, R.; Vagnozzi, A.; Valentini, S.

The light curve of the cataclismic variable ASASSN-18aan is studied using recent observations of the MC589 Observatory, giving an orbital Period and Epoch fully consistent with the data obtained after the discovery are in 2018. Archival data from ASASSN, ZTF and Gaia were used to check if its ares have a quasi-periodic behaviour. A recurrence time…

2023 Open European Journal on Variable Stars
Gaia 0
T Tauri stars in the SuperWASP and NSVS surveys II. Spectral modelling
DOI: 10.1093/mnras/stad2133 Bibcode: 2023MNRAS.524.3582H

Munari, U.; Smalley, B.; Kundra, E. +9 more

We present results from long-term spectroscopic monitoring of 21 T-Tauri stars located in the Taurus-Auriga star-forming region (SFR). We combine medium and high-dispersion Echelle spectroscopy obtained at the Stará Lesná, Skalnaté Pleso (both in Slovakia), and Tautenburg (Germany) observatories with low-resolution flux-calibrated spectra from Asi…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 0
Selection of Compton-thick AGN from a hard photometric sample using XMM-Newton observations
DOI: 10.1093/mnras/stad2425 Bibcode: 2023MNRAS.525.5080M

Guainazzi, Matteo; Mostafa, Reham; Ibrahim, Alaa

We present a selection technique to detect Compton-thick (CT) active galactic nuclei (AGNs) in the 3XMM/SDSS-DR7 cross-correlation. A subsample of 3481 X-ray sources that are detected in the hard band (2-8 keV) and have photometric redshifts constitute our parent sample. We first applied an automated spectral-fitting procedure to select highly abs…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
Study of the X-ray properties of radio sources, based on NVSS catalogue
DOI: 10.52526/25792776-23.70.1-88 Bibcode: 2023CoBAO..70...88P

Mickaelian, A. M.; Abrahamyan, H. V.; Paronyan, G. M. +4 more

An identification of radio sources from the NVSS list with ROSAT X-ray sources was made as well as also with optical objects from SDSS DR 16. We have tried to find the connection between the fluxes of different wave ranges, for different types of objects. We also have tried to find the relationship between the sizes and polarization angles of sour…

2023 Communications of the Byurakan Astrophysical Observatory
XMM-Newton 0
HST proper motions on the far side of the Galactic bar-data
DOI: 10.1093/mnras/stad1911 Bibcode: 2023MNRAS.524..224S

Clarkson, William I.; Rich, R. Michael; Kunder, Andrea +10 more

This is the third paper in a series that attempts to observe a clear signature of the Galactic bar/bulge using kinematic observations of the bulge stellar populations in low foreground extinction windows. We report on the detection of ~100 000 new proper motions in four fields covering the far side of the Galactic bar/bulge, at negative longitudes…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 0