Search Publications

Assessment of the cosmic distance duality relation using Gaussian process
DOI: 10.1093/mnras/stab1054 Bibcode: 2021MNRAS.504.3938M

Mukherjee, Ankan; Mukherjee, Purba

Two types of distance measurement are important in cosmological observations, the angular diameter distance dA and the luminosity distance dL. In this work, we carried out an assessment of the theoretical relation between these two distance measurements, namely the cosmic distance-duality relation, from type Ia supernova (SN-…

2021 Monthly Notices of the Royal Astronomical Society
eHST 26
New optically identified supernova remnants in the Large Magellanic Cloud
DOI: 10.1093/mnras/staa3382 Bibcode: 2021MNRAS.500.2336Y

Maitra, Chandreyee; Sasaki, Manami; Alsaberi, Rami Z. E. +20 more

We present a new optical sample of three Supernova Remnants (SNRs) and 16 Supernova Remnant (SNR) candidates in the Large Magellanic Cloud (LMC). These objects were originally selected using deep H α, [S II], and [O III] narrow-band imaging. Most of the newly found objects are located in less dense regions, near or around the edges of the LMC's ma…

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
First Solar Orbiter observation of the Alfvénic slow wind and identification of its solar source
DOI: 10.1051/0004-6361/202140938 Bibcode: 2021A&A...656A..21D

André, N.; Fedorov, A.; Livi, S. +27 more

Context. Turbulence dominated by large-amplitude, nonlinear Alfvén-like fluctuations mainly propagating away from the Sun is ubiquitous in high-speed solar wind streams. Recent studies have demontrated that slow wind streams may also show strong Alfvénic signatures, especially in the inner heliosphere.
Aims: The present study focuses on the c…

2021 Astronomy and Astrophysics
SolarOrbiter 26
Detectability of biosignatures on LHS 1140 b
DOI: 10.1051/0004-6361/202039663 Bibcode: 2021A&A...647A..48W

Rauer, Heike; Sousa-Silva, Clara; Wunderlich, Fabian +4 more

Context. Terrestrial extrasolar planets around low-mass stars are prime targets when searching for atmospheric biosignatures with current and near-future telescopes. The habitable-zone super-Earth LHS 1140 b could hold a hydrogen-dominated atmosphere, and is an excellent candidate for detecting atmospheric features.
Aims: In this study we inv…

2021 Astronomy and Astrophysics
Gaia eHST 26
A Study of the Photometric and Spectroscopic Variations of the Prototypical FU Orionis-type Star V1057 Cyg
DOI: 10.3847/1538-4357/ac04b3 Bibcode: 2021ApJ...917...80S

Cseh, B.; Kriskovics, L.; Pál, A. +19 more

Among the low-mass pre-main sequence stars, a small group called FU Orionis-type objects (FUors) are notable for undergoing powerful accretion outbursts. V1057 Cyg, a classical example of an FUor, went into outburst around 1969-1970, after which it faded rapidly, making it the fastest-fading FUor known. Around 1995, a more rapid increase in fading…

2021 The Astrophysical Journal
Gaia Herschel ISO 26
ALMA CO observations of a giant molecular cloud in M 33: Evidence for high-mass star formation triggered by cloud-cloud collisions
DOI: 10.1093/pasj/psaa045 Bibcode: 2021PASJ...73S..62S

Tokuda, Kazuki; Tachihara, Kengo; Sasaki, Manami +14 more

We report the first evidence for high-mass star formation triggered by collisions of molecular clouds in M 33. Using the Atacama Large Millimeter/submillimeter Array, we spatially resolved filamentary structures of giant molecular cloud 37 in M 33 using 12CO(J = 2-1), 13CO(J = 2-1), and C18O(J = 2-1) line emission …

2021 Publications of the Astronomical Society of Japan
Gaia eHST 26
Vortex-like kinematic signal, spirals, and beam smearing effect in the HD 142527 disk
DOI: 10.1051/0004-6361/202040089 Bibcode: 2021A&A...650A..59B

Pinte, C.; Ménard, F.; van der Plas, G. +8 more

Vortices are one of the most promising mechanisms to locally concentrate millimeter dust grains and allow the formation of planetesimals through gravitational collapse. The outer disk around the binary system HD 142527 is known for its large horseshoe structure with azimuthal contrasts of ~3-5 in the gas surface density and of ~50 in the dust. Usi…

2021 Astronomy and Astrophysics
Gaia 26
A magnetic reconnection model for hot explosions in the cool atmosphere of the Sun
DOI: 10.1051/0004-6361/202039239 Bibcode: 2021A&A...646A..88N

Ni, Lei; Chen, Yajie; Lin, Jun +2 more

Context. Ultraviolet (UV) bursts and Ellerman bombs (EBs) are transient brightenings observed in the low solar atmospheres of emerging flux regions. Magnetic reconnection is believed to be the main mechanism leading to formation of the two activities, which are usually formed far apart from each other. However, observations also led to the discove…

2021 Astronomy and Astrophysics
IRIS 26
Stellar Superflares Observed Simultaneously with Kepler and XMM-Newton
DOI: 10.3847/1538-4357/abf569 Bibcode: 2021ApJ...912...81K

Kolotkov, Dmitrii Y.; Kuznetsov, Alexey A.

Solar and stellar flares are powerful events that produce intense radiation across the electromagnetic spectrum. Multiwavelength observations are highly important for understanding the nature of flares, because different flare-related processes reveal themselves in different spectral ranges. To study the correlation between thermal and nonthermal …

2021 The Astrophysical Journal
XMM-Newton 26
A tidally tilted sectoral dipole pulsation mode in the eclipsing binary TIC 63328020
DOI: 10.1093/mnras/stab336 Bibcode: 2021MNRAS.503..254R

Handler, G.; Vanderburg, A.; Saio, H. +13 more

We report the discovery of the third tidally tilted pulsator, TIC 63328020. Observations with the TESS satellite reveal binary eclipses with an orbital period of 1.1057 d, and δ Scuti-type pulsations with a mode frequency of 21.09533 d-1. This pulsation exhibits a septuplet of orbital sidelobes as well as a harmonic quintuplet. Using th…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 26