A dataset provided by the European Space Agency

Name: A New Class of Massive Spiral Galaxies with High HI Masses
Published: 2018-01-04T23:00:00Z

Proposal ID	078235
Title	A New Class of Massive Spiral Galaxies with High HI Masses
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782350301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782350501
DOI	https://doi.org/10.5270/esa-g9uvfnm
Principal Investigator, PI	Prof Joel Bregman
Abstract	The most extensive HI survey, obtained with Arecibo, revealed a new category ofspiral galaxy in the local volume: massive spirals with a gaseous contentcomparable the stellar mass. These galaxies have high spin parameters, which maybe slowing the conversion of gas into stars. The gaseous disks are regular,suggesting that they arise from a radiatively cooling hot galactic halo that isparticularly massive and X-ray luminous. These may be local analogs to theactive hot mode accretion process that was common at z ~ 1-3 but is rare today.We propose the first X-ray observations of this newly recognized class ofgalaxies.
Publications	A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-11-26T12:50:00Z/2016-12-05T01:07:23Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2018-01-04T23:00:00Z
Keywords	"gaseous dis", "stellar mass", "local volume", "xray luminous", "recognized class", "massive spiral galaxy", "massive spirals", "spiral galaxy", "hi masses", "spin parameters", "local analogs", "gaseous content comparable", "extensive hi survey"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Joel Bregman, 2018, 'A New Class of Massive Spiral Galaxies with High HI Masses', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-g9uvfnm